07010138587|Happy New Year|OC|Other|no|January 1, 2007|no 07011529590|Spectroscopy of SMC Wolf-Rayet Stars Suggests that Wind-Clumping does not Depend on Ambient Metallicity|author{S.V. Marchenkoaltaffilmark{1}, C. Foellmialtaffilmark{2,3}, A.F.J. Moffataltaffilmark{4}, F. Martinsaltaffilmark{5}, J.-C. Bouretaltaffilmark{6}, E. Depagnealtaffilmark{3,7}}|Manuscript has been accepted|ApJL|January 15, 2007|http://gemini.tccw.wku.edu:8080/~sergey/ms.pdf 07011877423|Hot star wind models with new solar abundances|Jiri Krticka (1), Jiri Kubat (2)|Manuscript has been accepted|A&A Letters|January 18, 2007|http://xxx.lanl.gov/abs/astro-ph/0701411 07011955912|Constraining the fundamental parameters of the O-type binary|H. Sana^{1,2}, G. Rauw^{1} and E. Gosset^{1}|Manuscript has been accepted|Accepted by ApJ|January 19, 2007|http://arxiv.org/abs/astro-ph/0701574 07012659268|HV 11423: The Coolest Supergiant in the SMC|Philip Massey (1), Emily M. Levesque (2), K. A. G. Olsen (3), Bertrand Plez (4), B. A. Skiff (1)|Manuscript has been accepted|ApJ, in press|January 26, 2007|http://www.lowell.edu/users/massey/hv11423.pdf.gz 07020616512|On the co-existence of chemically peculiar Bp stars, slowly pulsating B stars and constant B stars in the same part of the H-R diagram|M. Briquet (1), S. Hubrig (2), P. De Cat (3), C. Aerts (1,4), P. North (5), and M. Scholler (2)|Manuscript has been accepted|Accepted for publication in Astronomy & Astrophysics on 29/01/2007|February 6, 2007|http://arxiv.org/abs/astro-ph/0702111 07020666010|Discovery of magnetic fields in three He variable Bp stars with He and Si spots|M. Briquet (1), S. Hubrig (2), M. Scholler (2), and P. De Cat (3)|Manuscript has been accepted|Astronomische Nachrichten, Vol.328, Issue 1, p.41-45|February 6, 2007|http://arxiv.org/pdf/astro-ph/0610537 0702066417|Near-IR imaging of Galactic massive clusters: Westerlund 2|J. Ascenso$^{1,2}$, J. Alves$^3$, Y. Beletsky$^4$, M. T. V. T. Lago$^{1,2}$|Manuscript has been accepted|A&A, in press|February 6, 2007|http://www.astro.up.pt/investigacao/ficheiros/175.pdf 07020934121|A Survey of Local Group Galaxies Currently Forming Stars: II. UBVRI Photometry of Stars in Seven Dwarfs|Philip Massey (1); K. A. G. Olsen (2); Paul W. Hodge (3); George H. Jacoby (4); Reagin T. McNeil (5); R. C. Smith (2); Shay B. Strong (6)|Manuscript has been accepted|Astronomical Journal, in press|February 9, 2007|http://www.lowell.edu/users/massey/dwarfs.pdf.gz 07021275367|Spectral atlas of massive stars around He I 10830 A|J. H. Groh (1), A. Damineli (1), F. Jablonski (2)|Manuscript has been accepted|Astronomy & Astrophysics, in press|February 12, 2007|http://arxiv.org/abs/astro-ph/0702169 07021594767|Direct constraint on the distance of y2 Velorum from AMBER/VLTI observations|F. Millour (1,2), R. G. Petrov (2), O. Chesneau (3), D. Bonneau (3), L. Dessart (13) and the AMBER consortium (1,2,3,4,5,6,7,8,9,10,11,12,14,15,16,17)|Manuscript has been accepted|DOI: 10.1051/0004-6361:20065408|February 15, 2007|http://fr.arxiv.org/abs/astro-ph/0610936 07021575227|First detection of phase-dependent colliding wind X-ray emission outside the Milky Way|Yael Naze (1), Michael F. Corcoran (2), Gloria Koenisgberger (3), Anthony F.J. Moffat (4)|Manuscript has been accepted|accepted by ApJ (letters)|February 15, 2007|http://arxiv.org/abs/astro-ph/0702403 07021540875|X-ray Spectral Variation of Eta Carinae through the 2003 X-ray Minimum|Kenji Hamaguchi(1,2), Michael F. Corcoran(1,2), Theodore Gull(3), Kazunori Ishibashi(4), Julian M. Pittard(5), D. John Hillier(6), Augusto Damineli(7), Kris Davidson(8), Krister E. Nielsen(3,9), Gladys Vieira Kober(3,9)|Manuscript has been accepted|ApJ in press|February 15, 2007|http://arxiv.org/abs/astro-ph/0702409 07021526178|Optically Observable Zero-Age Main-Sequence O Stars|Nolan R. Walborn|Conference proceedings|STScI 2006 May Symposium, Massive Stars:
Pop III and GRBs to the Milky Way, ed. M. Livio & E. Villaver,
(Cambridge University Press)|February 15, 2007|http://arxiv.org/abs/astro-ph/0701573 07022037188|Physical Orbit for Lambda Virginis and a Test of Stellar Evolution Models|M. Zhao $^1$, J. D. Monnier $^1$, G. Torres $^2$, A. F. Boden $^3$, A. Claret $^4$, R. Millan-Gabet $^3$, E. Pedretti $^1$, J.-P. Berger $^5$, W. A. Traub $^2$, F. P. Schloerb $^6$, N. P. Carleton $^2$, P. Kern $^5$, M. G. Lacasse $^2$, F. Malbet $^5$, K. Perraut $^5$|Manuscript has been accepted|ApJ, 658 (in press, 2007 March 20)|February 20, 2007|http://arxiv.org/abs/astro-ph/0612135 07022372344|The stellar upper mass limit in the solar neighborhood|J. Maíz Apellániz, Nolan R. Walborn, N. I. Morrell, E. P. Nelan, V. S. Niemela, P. Benaglia, A. Sota|Conference proceedings|To appear in Massive Stars: Fundamental Parameters and Circumstellar Interactions|February 23, 2007|http://xxx.arxiv.org/abs/astro-ph/0702514 070223824|Towards using optical/NIR photometry to measure the temperature of O stars|J. Maíz Apellániz & A. Sota|Conference proceedings|To appear in Massive Stars: Fundamental Parameters and Circumstellar Interactions|February 23, 2007|http://xxx.arxiv.org/abs/astro-ph/0702516 07022741625|Eclipsing Binary System WN3(h)+O5V BAT99-129: Analysis of the MACHO Light Curve and the Parameters of the Components|I.I. Antokhin, A.M. Cherepashchuk|Manuscript has been accepted|Astronomy Reports|February 27, 2007|http://arxiv.org/abs/astro-ph/0702658 07030123313|The 3D Morphology of VY Canis Majoris. I The Kinematics of the Ejecta|Roberta M. Humphreys, L. Andrew Helton, Terry J. Jones|Manuscript has been accepted|Astronomical Journal|March 1, 2007| 07030235203|The 3D Morphology of VY Canis Majoris II: Polarimetry and the Line-of-Sight Distribution of the Ejecta|Terry Jay Jones, Roberta M. Humphreys, and L. Andrew Helton (1) and Changfeng Gui and Xiang Huang (2)|Manuscript has been accepted|Astronomical Journal|March 2, 2007| 07030267055|The Galactic O Star Catalog V.2.0|Alfredo Sota (1), Jesús Maíz Apellániz (2), Nolan R. Walborn (1), and Raquel Y. Shida (3)|Conference proceedings|"Massive Stars: Fundamental Parameters and Circumstellar Interactions"
Carilo, Argentina
December 11-14, 2006|March 2, 2007|http://arxiv.org/abs/astro-ph/0703005 0703051744|Central Stars of Planetary Nebulae in the Galactic Bulge|P.J.N. Hultzsch, J. Puls, R.H. Mendez, A.W.A. Pauldrach, R.-P. Kudritzki, T.L. Hoffmann, J.K. McCarthy|Manuscript has been accepted|A&A, accepted; astro-ph/0702755|March 5, 2007|http://www.usm.uni-muenchen.de/people/puls/papers/cspn.pdf 07030636820|An XMM-Newton view of the young open cluster NGC 6231 III. Optically faint X-ray sources|H. Sana$^{1,2}, G. Rauw$^1$, H. Sung$^3$, E. Gosset$^1, J.-M. Vreux$^1$|Manuscript has been accepted|Accepted by MNRAS|March 6, 2007|http://arxiv.org/abs/astro-ph/0703104 07030992071|A New Numerical Method for Solving Radiation Driven Winds from Hot Stars|Michel Cure (1), Diego F. Rial (1,2)|Manuscript has been accepted|Accepted for publication in Astronomische Nachrichten / Astronomical Notes|March 9, 2007|http://xxx.lanl.gov/abs/astro-ph/0703148 07031081201|Stellar and wind properties of massive stars in the central parsec of the Galaxy|F. Martins (1), R. Genzel (1,2), D.J. Hillier (3), F. Eisenhauer (1), T. Paumard (1,4), S. Gillessen (1), T. Ott (1), S. Trippe (1)|Manuscript has been accepted|A&A acceoted|March 10, 2007|http://arxiv.org/abs/astro-ph/0703211 07031288763|Fourier method in the determination of rotational velocities in OB stars|S. Simón-Díaz (1,2), A. Herrero (1,3)|Manuscript has been accepted|A&A|March 12, 2007|http://xxx.lanl.gov/abs/astro-ph/0703216 07031639688|VLT/NACO near-infrared imaging and spectroscopy of N159-5 in the LMC HII complex N159|G. Testor (1), J.L. Lemaire (2), L.Kristensen(2), D. Field (3), S. Diana (2)|Manuscript has been accepted|A&A|March 16, 2007|not available 07032185119|Detection of variable Si~II, Mn~II and Fe~II emission lines in the magnetic Bp star a~Centauri|S. Hubrig$^1$, J.F. Gonzalez$^2$|Manuscript has been accepted|Accepted for publication in A&A|March 21, 2007|http://arxiv.org/abs/astro-ph/0703229 07032684713|A Clumping Independent Diagnostic of Stellar Mass-loss Rates: Rapid Clump Destruction in Adiabatic Colliding Winds|J. M. Pittard|Manuscript has been accepted|Accepted by ApJL|March 26, 2007|astro-ph/0703617 07032843054|Testing the predicted mass-loss bi-stability jump at radio wavelengths|P. Benaglia(1,2), J. S. Vink(3,4), J. Marti(5), J. Maiz Apellaniz(6,7), B. Koribalski(8), and P.A. Crowther(9)|Manuscript has been accepted|The paper is recommended for publication in A&A (astro-ph/0703577)|March 28, 2007|www.iar.unlp.edu.ar/garra/garra-pb.html 07042095819|Modelling the clumping-induced polarimetric variability of hot star winds|Ben Davies(^1,2), Jorick S. Vink(^3,4,5), René D. Oudmaijer(^2)|Manuscript has been accepted|Accepted for publication in A&A|April 20, 2007|http://www.cis.rit.edu/~bxdpci/7193accepted.pdf 07042470813|Constraining GRB progenitor models by probing Wolf-Rayet wind geometries in the Large Magellanic Cloud|Jorick S. Vink|Manuscript has been accepted|A&A, astro-ph/0704.2690|April 24, 2007|http://www.arm.ac.uk/~jsv/ 07042492988|Luminous blue variables as the progenitors of supernovae with quasi-periodic radio modulations|Rubina Kotak$^1,2$, Jorick S Vink $^3,4$|Manuscript has been accepted|2006, A&A 460L, 5|April 24, 2007| 07050947627|The WR population predicted by massive single star and by massive binary evolution|D. Vanbeveren, J. Van Bever, H. Belkus|Manuscript has been accepted|ApJ Letters|May 9, 2007|astro-ph/0703796 07051196196|Wind-wind collision in the eta Carinae binary system - III.The He II 4686 line profile|Z. Abraham (1) & D. Falceta-Goncalves (1,2)|Manuscript has been accepted|MNRAS|May 11, 2007|http://xxx.lanl.gov/abs/astro-ph/0703695 07051372188|On the optical counterpart of NGC300 X-1 and the global Wolf-Rayet content of NGC300|Paul A Crowther (1), S. Carpano (2), L.J. Hadfield (1), A.M.T. Pollock (2)|Manuscript has been accepted|A&A Letters in press|May 13, 2007|http://arxiv.org/abs/0705.1544 07051431091|Erratum: An overview of the photometric events, trends and brightenings of $eta$~Carinae}|A. M. van Genderen$^1$, C.~Sterken$^{2}$ , W. H. Allen$^3$ and W. S. G. Walker$^4$|Manuscript has been accepted|The Journal of Astronomical data 13, 1 2007|May 14, 2007|ADS 07061174189|Late-Type Red Supergiants: Too Cool for the Magellanic Clouds?|Emily M. Levesque, Philip Massey, K. A. G. Olsen, Bertrand Plez|Manuscript has been accepted|ApJ, in press|June 11, 2007|http://xxx.lanl.gov/abs/0705.3431 07061989692|Models for Massive Stellar Populations with Rotation|Gerardo A. Vazquez, Claus Leitherer, Daniel Schaerer, Georges Meynet, Andre Maeder|Manuscript has been accepted|Astrophysical Journal, 2007, 663, 995|June 19, 2007|http://arxiv.org/abs/astro-ph/0703699 07063011282|An Extensive Collection of Stellar Wind X-ray Source Region Emission Line Parameters, Temperatures, Velocities, and Their Radial Distributions as Obtained from Chandra Observations of 17 OB Stars|Wayne L. Waldron (1), Joseph P. Cassinelli (2)|Manuscript has been accepted|ApJ, 668, in press|June 30, 2007| 07071363543|INTEGRAL-ISGRI observations of the CygOB2 region: searching for hard X-ray point sources in a region containing several non-thermal emitting massive stars|De Becker M.$^1$, Rauw G.$^1$, Pittard J.M.$^2$, Sana H.$^3$, Stevens I.R.$^4$, Romero G.E.$^{5,6}$|Manuscript has been accepted|Astronomy and Astrophysics|July 13, 2007|http://arxiv.org/abs/0707.2005 07071858272|Neon Abundances from a Spitzer/IRS Survey of Wolf-Rayet Stars|R Ignace^1, J Cassinelli^2, G Tracy^2, E Churchwell^2, H Lamers^3|Manuscript has been accepted|Astrophysical Journal|July 18, 2007|http://www.etsu.edu/physics/ignace/pubs.html 07073041594|Orbital effects on the light curves of eta Car, BP Cru, and other eccentric binaries|van Genderen, A.M.; Sterken, C.|Manuscript has been accepted|IBVS No. 5782 2007|July 30, 2007|http://www.konkoly.hu/cgi-bin/IBVS?5782 07080144698|X-Rays From Massive OB Stars: Thermal Emission From Radiative Shocks|Svetozar A. Zhekov (1) and Francesco Palla (2)|Manuscript has been accepted|MNRAS|August 1, 2007|http://arxiv.org/abs/0708.0085 07080654489|A massive cluster of Red Supergiants at the base of the Scutum-Crux arm|Ben Davies (1), Don F. Figer (1), Rolf-Peter Kudritzki (2), John MacKenty (3), Francisco Najarro (4) and Artemio Herrero (5)|Manuscript has been accepted|To appear in ApJ|August 6, 2007|http://www.cis.rit.edu/~bxdpci/RSGC2.pdf 07080728051|The Role of Evolutionary Age and Metallicity in the Formation of Classical Be Circumstellar Disks II. Assessing the Evolutionary Nature of Candidate Disk Systems|John P. Wisniewski$^1$, Karen S. Bjorkman$^2$, Antonio M. Magalh~aes$^3$, Jon E. Bjorkman$^2$, Marilyn R. Meade$^4$, & Antonio Pereyra$^3$|Manuscript has been accepted|ApJ|August 7, 2007|http://arxiv.org/abs/0708.0651 07080848700|Discovery of a New Dusty B[e] Star in the Small Magellanic Cloud|John P. Wisniewski$^1$, Karen S. Bjorkman$^2$, Jon E. Bjorkman$^2$, and Mark Clampin$^1$|Manuscript has been accepted|ApJ|August 8, 2007|http://arxiv.org/abs/0708.1030 07081662969|Integral-Field Spectroscopy of the Post Red Supergiant IRC +10420: evidence for an axi-symmetric wind|Ben Davies (1,2), René D. Oudmaijer (2), Kailash C. Sahu (3)|Manuscript has been accepted|To appear in ApJ|August 16, 2007|http://www.cis.rit.edu/~bxdpci/pubs.html 07081674390|Circumstellar Magnetic Field Diagnostics from Line Polarization|Richard Ignace (1) and Kenneth G. Gayley (2)|Conference proceedings|to appear in the proceedings of Clumping in Hot Star Winds|August 16, 2007|http://lanl.arxiv.org/abs/0708.1942 07082084525|Physical Properties of Red Supergiants|Philip Massey (1), Bertrand Plez (2), Emily M. Levesque (3), K. A. G. Olsen (4), David R Silva (5), and Geoffery C. Clayton (6)|Conference proceedings|to appear in The Biggest, Baddest, Coolest Stars, ASP Conf Series, ed. D. Luttermoser, B. Smith, and R. Stencel|August 20, 2007|http://www.lowell.edu/users/massey/tennmasseyp.pdf 07082174816|The Coolest Stars in the Clouds: Unusual Red Supergiants in the Magellanic Clouds|Emily M. Levesque (1), Philip Massey (2), K. A. G. Olsen (3), Bertrand Plez (4)|Conference proceedings|to appear in The Biggest, Baddest, Coolest Stars, ASP Conf Series, ed. D. Luttermoser, B. Smith, and R. Stencel|August 21, 2007|http://ifa.hawaii.edu/~emsque/RSGs/levesquee.pdf 07082370179|The Struve-Sahade effect in the optical spectra of O-type binaries I. Main-sequence systems|N. Linder (1), G. Rauw (1), H. Sana (2), M. De Becker (1), E. Gosset (1)|Manuscript has been accepted|A & A, in press|August 23, 2007|http://www.arxiv.org/abs/0708.3005 07082738116|On the X-ray and optical properties of the Be star HD 110432: a very hard-thermal X-ray emitter|Raimundo LOPES DE OLIVEIRA Filho (1,2), Christian MOTCH (2), Myron A. SMITH (3), Ignacio NEGUERUELA (4) and Jose M. TORREJON (4)|Manuscript has been accepted|A&A, in press|August 27, 2007|http://arxiv.org/abs/astro-ph/0701767 07090478709|The impact of reduced mass loss rates on the evolution of massive stars|Raphael HIRSCHI|Conference proceedings|proceedings for a review talk at the International Workshop on "CLUMPING in Hot-Star Winds", 18. - 22. June 2007, Potsdam, Germany. To be published electronically by the University of Potsdam (Universitaets-Verlag), Editors: Wolf-Rainer Hamann, Achim Feldmeier and Lidia Oskinova|September 4, 2007|http://arxiv.org/abs/0709.0392 07090523105|A Rigid-Field Hydrodynamics approach to modeling the magnetospheres of massive stars|R. H. D. Townsend, S. P. Owocki, A. ud-Doula|Manuscript has been accepted|MNRAS, in press|September 5, 2007|http://arxiv.org/pdf/0709.0694 07090618832|Techniques for simulating radiative transfer through porous media|Rich Townsend|Conference proceedings|To appear in proceedings of "Clumping in Hot Star Winds" conference (Potsdam, Germany, June 2007)|September 6, 2007|http://arxiv.org/pdf/0709.0860 07090689043|The coupling between pulsation and mass loss in massive stars|Rich Townsend|Conference proceedings|To appear in proceedings of "Unsolved Problems in Stellar Physics" conference (Cambridge, UK, July 2007)|September 6, 2007|http://arxiv.org/pdf/0709.0761 07090964985|A Survey of Local Group Galaxies Currently Forming Stars: III. A Search for Luminous Blue Variables and Other Halpha Emission-Lined Stars|Philip Massey (1), Reagin T. McNeill (1,2), K. A. G. Olsen (3), Paul W. Hodge (4), Cynthia Blaha (5), George H. Jacoby (6), R. C. Smith (3), and Shay B. Strong (7)|Manuscript has been accepted|Astronomical Journal, in press|September 9, 2007|http://www.lowell.edu/users/massey/has.pdf.gz 07091055008|The investigation of particle acceleration in colliding-wind massive binaries with SIMBOL-X.|De Becker M.^1, Rauw G.^1, Pittard J.M.^2, Blomme R.^3, Romero G.E.^4, Sana H.^5, Stevens I.R.^6|Conference proceedings|To appear in the proceedings of the workshop "Simbol-X: the hard X-ray universe in focus", held in Bologna, Italy (14-16 May 2007)|September 10, 2007|http://arxiv.org/abs/0709.1033 07091112615|Colliding Stellar Wind Models with Nonequilibrium Ionization: X-rays from WR 147|Svetozar A. Zhekov|Manuscript has been accepted|MNRAS|September 11, 2007|http://arxiv.org/abs/0709.1686 07091928659|The RMS Survey: Mid-Infrared Observations of Candidate Massive YSOs in the Southern Hemisphere|J.C. Mottram$^1$, M.G. Hoare$^1$, S.L. Lumsden$^1$, R.D. Oudmaijer$^1$, J.S. Urquhart$^1$, T.L. Sheret$^1$, A.J. Clarke$^1$, J. Allsopp$^2$|Manuscript has been accepted|Accepted by Astronomy and Astrophysics|September 19, 2007| 07092548537|Non-thermal emission processes in massive binaries|Michaël De Becker|Manuscript has been accepted|Astronomy & Astrophysics Review, in press|September 25, 2007|http://adsabs.harvard.edu/doi/10.1007/s00159-007-0005-2 07100351153|The B and Be Star Population of NGC 3766|M. Virginia McSwain$^1$, Wenjin Huang$^2$, Douglas R. Gies$^3$, Erika D. Grundstrom$^4$, Richard H. D. Townsend$^5$|Manuscript has been accepted|to appear in the Astrophysical Journal|October 3, 2007|astro-ph/0710.0137 07101319403|X-ray Emission from Magnetically Torqued Disks of Oe/Be Stars|Q. Li (1,3), J.P. Cassinelli (2), J. C. Brown (3), W. L. Waldron (4), N. A. Miller (5)|Manuscript has been accepted|ApJ in press.|October 13, 2007|http://arxiv.org/abs/astro-ph/0710.2633 07102690346|Modeling the line variations from the wind-wind shock emissions of WR30a|Falceta-Goncalves, D. (1), Abraham, Z. (2) and Jatenco-Pereira, V. (2)|Manuscript has been accepted|accepted for publication in the MNRAS|October 26, 2007|http://arxiv.org/abs/0710.0662 07103138371|Super-AGB stars and the fine line between White Dwarf or Supernova|Royal Astronomical Society Specialist Discussion Meeting|Other|Meeting announcement|October 31, 2007|http://www.astro.keele.ac.uk/e-stars/ras2008/ras2008.html 07110522651|The most massive stars in the Arches cluster|F. Martins (1), D.J. Hillier (2), T. Paumard (3), F. Eisenhauer (1), T. Ott (1), R. Genzel (1,4)|Manuscript has been accepted|A&A accepted|November 5, 2007|http://arxiv.org/abs/0711.0657 07110989096|Bright OB stars in the Galaxy -IV. Stellar and wind parameters of early to late B supergiants|N. Markova$^1$, J. Puls$^2$|Manuscript has been accepted|A&A, in press|November 9, 2007|http://www.usm.uni-muenchen.de/people/puls/papers/GalBSg.pdf 0711129875|Evolution towards the critical limit and the origin of Be stars|S. Ekstr"om, G. Meynet, A. Maeder & F. Barblan|Manuscript has been accepted|Astronomy and Astrophysics|November 12, 2007|http://arxiv.org/abs/0711.1735 07112217895|XMM-Newton X-ray study of early type stars in the Carina OB1 association|Igor.I.Antokhin (1,2,3), Gregor Rauw (2), Jean-Marie Vreux (2), Karel A. van der Hucht (4,5), John C. Brown (3)|Manuscript has been accepted|Accepted by Astronomy and Astrophysics|November 22, 2007|http://arxiv.org/abs/0711.3612 07112679430|Phase-dependent X-ray observations of the beta Lyrae system: No eclipse in the soft band|R Ignace$^1$, L M Oskinova$^2$, W L Waldron$^3$, J L Hoffman$^4$, W-R Hamann$^5$|Manuscript has been accepted|to appear as a Letter in A&A|November 26, 2007|astroph/0711.3954 07112735249|Carbon abundances of early B-type stars in the solar vicinity. Non-LTE line-formation for C II/III/IV and self-consistent atmospheric parameters|M.F. Nieva (1,2), N. Przybilla (1)|Manuscript has been accepted|A&A|November 27, 2007|http://arxiv.org/abs/0711.3783 07112784107|Neglecting the porosity of hot-star winds can lead to underestimating mass-loss rates|L.M. Oskinova, W.-R. Hamann, and A. Feldmeier|Manuscript has been accepted|DOI: 10.1051/0004-6361:20066377|November 27, 2007|astro-ph/0704.2390 07112999648|The cool supergiant population of the massive young star cluster RSGC1|Ben Davies (RIT), Don F. Figer (RIT), Casey J. Law (Amsterdam), Rolf-Peter Kudritzki (IfA, Hawaii), Francisco Najarro (CSIC, Madrid), Artemio Herrero (IAC, Spain), John W. MacKenty (STScI)|Manuscript has been accepted|astro-ph/0711.4757|November 29, 2007|http://arxiv.org/abs/0711.4757v1 0712061459|Quantitative analysis of resolved X-ray emission line profiles of O stars|David H. Cohen (1), Maurice A. Leutenegger (2), Richard H. D. Townsend (3)|Conference proceedings|Appearing in "Clumping in Hot Star Winds," eds. Hamann, Feldmeier, & Oskinova, Potsdam: Univ.-Verl., 2007|December 6, 2007|http://astro.swarthmore.edu/~cohen/Papers/cohen_potsdam.pdf 07121465662|The periodicity of the eta Carinae events|A. Damineli (1), M. F. Corcoran (3,4), D. J. Hillier (2), O. Stahl(5), R. S. Levenhagen (1), N.V. Leister (1), J. H. Groh (1), M. Teodoro (1), J. F. Albacete Colombo (6), F. Gonzalez (7), J. Arias (8), H. Levato (7), M. Grosso (7), N. Morrell (9), R. Gamen (7), G.Wallerstein (10), V. Niemela (11)|Manuscript has been accepted|MNRAS|December 14, 2007| 07121721220|Dynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: II. The Effects of Field-Aligned Rotation|Asif ud-Doula^{1,2}, Stanley P. Owocki^1 and Richard H.D. Townsend^1|Manuscript has been accepted|MNRAS (in press)|December 17, 2007|http://shayol.bartol.udel.edu/massivewiki-media/publications/rotation.pdf 07121736685|The Massive Star Content of NGC 3603|Nicholas W. Melena (1), Philip Massey (1), Nidia I. Morrell (2), and Amanda M. Zangari (1,3)|Manuscript has been accepted|AJ, in press|December 17, 2007|http://www.lowell.edu/users/massey/n3603final.pdf 071223881|The circumstellar medium around a rapidly rotating, chemically homogeneously evolving, possible gamma-ray burst progenitor|Allard Jan van Marle(1,2), Norbert Langer(1), Sung-Chul Yoon(3), and Guillermo Garcia-Segura(4)|Manuscript has been accepted|Accepted for publication in Astronomy & Astrophysics|December 23, 2007|http://lanl.arxiv.org/abs/0711.4807