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相关论文: A New Galactic Wolf-Rayet Star in Centaurus

200 篇论文

In this paper we report the identification of two new Galactic O2 If*/WN6 stars (WR20aa and WR20c), in the outskirt of the massive young stellar cluster Westerlund 2. The morphological similarity between the near-infrared spectra of the new…

星系天体物理 · 物理学 2011-07-26 A. Roman-Lopes , R. H. Barba , N. I. Morrell

We provide line luminosities and spectroscopic templates of prominent optical emission lines of 133 Galactic Wolf-Rayet stars by exploiting Gaia DR3 parallaxes and optical spectrophotometry, and provide comparisons with 112 counterparts in…

太阳与恒星天体物理 · 物理学 2023-02-15 Paul A. Crowther , G. Rate , Joachim M. Bestenlehner

We report the detection of 3 additional Wolf-Rayet stars in the young cluster Westerlund 1. They were selected as emission-line star candidates based on 1 micron narrow-band imaging of the cluster carried out at OPD/LNA (Brazil), and then…

天体物理学 · 物理学 2009-11-11 J. H. Groh , A. Damineli , M. Teodoro , C. L. Barbosa

This paper gathers, from the literature and private communication, 72 new Galactic Population I Wolf-Rayet stars and 17 candidate WCLd stars, recognized and/or discovered after the publication of The VIIth Catalogue of Galactic Wolf-Rayet…

天体物理学 · 物理学 2008-11-26 Karel A. van der Hucht

Recent large scale Galactic Plane H$\alpha$ surveys allow a re-examination of the environs of Wolf-Rayet (WR) stars for the presence of a circumstellar nebula. Using the morphologies of WR nebulae known to be composed of stellar ejecta as a…

星系天体物理 · 物理学 2015-05-19 D. J. Stock , M. J. Barlow

We report the discovery of broad Wolf-Rayet emission lines in the Multiple Mirror Telescope (MMT) spectrum of the NW component of I Zw 18, the lowest-metallicity blue compact dwarf (BCD) galaxy known. Two broad Wolf-Rayet (W-R) bumps at the…

天体物理学 · 物理学 2014-10-13 Yuri I. Izotov , Craig B. Foltz , Richard F. Green , Natalia G. Guseva , Trinh X. Thuan

Wolf-Rayet stars (WR) have been detected in the NW region of the metal-poor starburst galaxy IZw 18. The integrated luminosity and FWHM of the bumps at 4650 A and 5808 A are consistent with the presence of a few individual stars of WC4 or…

天体物理学 · 物理学 2007-05-23 F. Legrand , D. Kunth , J. -R. Roy , J. M. Mas-Hesse , J. R. Walsh

We summarize the results of our four year survey searching for Wolf-Rayet (WR) stars in the Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC). Over the course of this survey we've discovered 15 new WRs and 12 Of-type stars. In…

太阳与恒星天体物理 · 物理学 2018-08-29 Kathryn F. Neugent , Philip Massey , Nidia Morrell

We report the discovery of a new Wolf-Rayet star in Aquila via detection of its circumstellar nebula (reminiscent of ring nebulae associated with late WN stars) using the Spitzer Space Telescope archival data. Our spectroscopic follow-up of…

太阳与恒星天体物理 · 物理学 2014-11-20 V. V. Gvaramadze , A. Y. Kniazev , W. -R. Hamann , L. N. Berdnikov , S. Fabrika , A. F. Valeev

We have obtained spectroscopic observations of the nebulae around seven Wolf-Rayet (WR) stars, four in the Milky Way (WR 8, 16, 18 and 40) and three in the LMC (BAT99-2, -11 and -38). They were observed using the ESO NTT with the EFOSC-2…

星系天体物理 · 物理学 2015-05-30 D. J. Stock , M. J. Barlow , R. Wesson

We present the most comprehensive and deepest X-ray study to date of the properties of the richest Wolf-Rayet (WR) population observed in a single stellar cluster, Westerlund 1 (Wd1). This work is based on 36 Chandra observations obtained…

We report the detection of WC stars in 5 Wolf-Rayet (WR) galaxies: He 2-10, NGC 3049, NGC 3125, NGC 5253 and Tol 89. The faint broad CIV5808 line requires sufficiently high S/N to be detected explaining the non-detection of this WC feature…

天体物理学 · 物理学 2007-05-23 Daniel Schaerer , Thierry Contini , Daniel Kunth

Context. A significant number of the Wolf-Rayet stars seem to be binary or multiple systems, but the nature of many of them is still unknown. Dedicated monitoring of WR stars favours the discovery of new systems. Aims. We explore the…

太阳与恒星天体物理 · 物理学 2015-06-15 A. Collado , R. Gamen , R. H. Barbá

The numbers and types of evolved massive stars found in nearby galaxies provide an exacting test of stellar evolution models. Because of their proximity and rich massive star populations, the Magellanic Clouds have long served as the…

太阳与恒星天体物理 · 物理学 2015-07-15 Philip Massey , Kathryn F. Neugent , Nidia Morrell

As part of a search for Wolf-Rayet (WR) stars in the Magellanic Clouds, we have discovered a new type of WR star in the Large Magellanic Cloud (LMC). These stars have both strong emission lines, as well as He ii and Balmer absorption lines…

太阳与恒星天体物理 · 物理学 2017-05-31 Kathryn F. Neugent , Philip Massey , D. John Hillier , Nidia I. Morrell

IC10 is the nearest starburst galaxy, as revealed both by its Halpha surface brightness and the large number of Wolf-Rayet stars (WRs) per unit area. The relative number of known WC- to WN-type WRs has been thought to be unusually high…

天体物理学 · 物理学 2009-11-07 Philip Massey , Shadrian Holmes

We report the serendipitous discovery of a heavily reddened Wolf-Rayet star that we name WR142b. While photometrically monitoring a cataclysmic variable, we detected weak variability in a nearby field star. Low-resolution spectroscopy…

We are conducting a high angular resolution imaging survey of Galactic Wolf-Rayet stars using the Wide Field and Planetary Camera 2 aboard the Hubble Space Telescope. We have found a small stellar cluster associated with the faint, close…

We present new identifications of infrared counterparts to the population of hard X-ray sources near the Galactic center detected by the Chandra X-ray Observatory. We have confirmed 16 new massive stellar counterparts to the X-ray…

星系天体物理 · 物理学 2014-11-20 Jon C. Mauerhan , Michael P. Muno , Mark R. Morris , Susan R. Stolovy , Angela S. Cotera

We present deep H$\alpha$ and [O III] images of the ejecta rich nebulosity associated with the suspected runaway and binary Wolf-Rayet star WR~71 (HD 143414). In H$\alpha$ emission, the nebula appears as a crescent shaped, broken ring of…

高能天体物理现象 · 物理学 2025-07-25 Robert A. Fesen , Manuel C. Peitsch , Martin R. Pugh , Bray Falls , Marcel Drechsler