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相关论文: Hot gas in the Wolf-Rayet nebula NGC3199

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We present deep XMM-Newton EPIC observations of the Wolf-Rayet (WR) bubble NGC6888 around the star WR136. The complete X-ray mapping of the nebula confirms the distribution of the hot gas in three maxima spatially associated with the caps…

太阳与恒星天体物理 · 物理学 2016-01-20 J. A. Toalá , M. A. Guerrero , Y. -H. Chu , S. J. Arthur , D. Tafoya , R. A. Gruendl

We discuss our most recent findings on the diffuse X-ray emission from Wolf-Rayet (WR) nebulae. The best-quality X-ray observations of these objects are those performed by XMM-Newton and Chandra towards S308, NGC2359, and NGC6888. Even…

高能天体物理现象 · 物理学 2015-11-04 J. A. Toalá , M. A. Guerrero , Y. -H. Chu , S. J. Arthur , R. A. Gruendl

A recent XMM-Newton observation (Zhekov 2014) has revealed diffuse X-ray emission inside the nebula NGC 2359 around the Wolf-Rayet star WR 7. Taking advantage of an improved point-source rejection and background subtraction, and a detailed…

太阳与恒星天体物理 · 物理学 2015-06-23 J. A. Toalá , M. A. Guerrero , Y. -H. Chu , R. A. Gruendl

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 report the serendipitous detection of the planetary nebula NGC 5315 by the Chandra X-ray Observatory. The Chandra imaging spectroscopy results indicate that the X-rays from this PN, which harbors a Wolf-Rayet (WR) central star, emanate…

天体物理学 · 物理学 2012-08-27 Joel Kastner , Rodolfo Montez, , Bruce Balick , Orsola De Marco

We present the results of Chandra X-ray Observatory (CXO) observations of the planetary nebulae (PNs) NGC 40 and Hen 2-99. Both PNs feature late-type Wolf-Rayet central stars that are presently driving fast ~1000 km/s, massive winds into…

天体物理学 · 物理学 2009-11-13 Rodolfo Montez , Joel H. Kastner , Orsola De Marco , Noam Soker

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

We present an analysis of the XMM-Newton observation of the wind-blown bubble NGC 2359. This is the first detection of this object in X-rays. The X-ray emission of NGC 2359 is soft and originates from a thermal plasma with a typical…

高能天体物理现象 · 物理学 2015-06-19 Svetozar A. Zhekov

We present Hubble Space Telescope WFPC2 images of a portion of the bright northeast rim of NGC 6888, the nebular shell physically associated with the Wolf-Rayet star HD 192163. The exposures are taken in the light of Halpha 6563, [O III]…

天体物理学 · 物理学 2009-10-31 Brian D. Moore , J. Jeff Hester , Paul A. Scowen

We summarize new X-ray detections of four nitrogen-type Wolf-Rayet (WR) stars obtained in a limited survey aimed at establishing the X-ray properties of WN stars across their full range of spectral subtypes. None of the detected stars is so…

太阳与恒星天体物理 · 物理学 2015-05-14 S. L. Skinner , S. A. Zhekov , M. Guedel , W. Schmutz , K. R. Sokal

We report the discovery of weak yet hard X-ray emission from the Wolf-Rayet (WR) star WR142 with the XMM-Newton X-ray telescope. Being of spectral subtype WO2, WR142 is a massive star in a very advanced evolutionary stage, short before its…

太阳与恒星天体物理 · 物理学 2009-11-13 L. M. Oskinova , W. -R. Hamann , A. Feldmeier , R. Ignace , Y. -H. Chu

We analyze Chandra observations of the Wolf-Rayet (WR) bubble NGC 6888. This WR bubble presents similar spectral and morphological X-ray characteristics to those of S 308, the only other WR bubble also showing X-ray emission. The observed…

太阳与恒星天体物理 · 物理学 2015-06-17 J. A. Toalá , M. A. Guerrero , R. A. Gruendl , Y. -H. Chu

We present the analysis of XMM-Newton archival observations towards the Wolf-Rayet (WR) bubble around WR16. Despite the closed bubble morphology of this WR nebula, the XMM-Newton observations show no evidence of diffuse emission in its…

太阳与恒星天体物理 · 物理学 2015-06-17 J. A. Toalá , M. A. Guerrero

We present XMM-Newton observations of the dusty Wolf-Rayet star WR 48a. This is the first detection of this object in X-rays. The XMM-Newton EPIC spectra are heavily absorbed and the presence of numerous strong emission lines indicates a…

太阳与恒星天体物理 · 物理学 2015-05-20 Svetozar A. Zhekov , Marc Gagne , Stephen L. Skinner

We present the discovery of extended X-ray emission from the planetary nebula (PN) NGC 5189 around the [WO1]-type WD 1330-657 with XMM-Newton. The X-ray-emitting gas fills the cavities detected in the Hubble Space Telescope [O III]…

太阳与恒星天体物理 · 物理学 2020-01-08 J. A. Toalá , R. Montez , M. Karovska

This work aims to search for the observational footprints of the interactions between the interstellar medium (ISM) and stellar winds in the Wolf-Rayet (WR) nebula NGC6888 in order to understand its ionization structure, chemical…

We report the serendipitous discovery of a ring nebula around a candidate Wolf-Rayet (WR) star, HBHA 4202-22, in Cygnus using the Spitzer Space Telescope archival data. Our spectroscopic follow-up observations confirmed the WR nature of…

We report the results of deep H$\alpha$ and [O III] images of the bright WN6/WC4 Wolf-Rayet star WR~8 (HD~62910). These data show considerably more surrounding nebulosity than seen in prior imaging. The brighter portions of the nebula span…

We have used the excellent sensitivity of XMM-Newton to obtain the first high-quality X-ray spectrum of a Wolf-Rayet (WR) star which is not known to be a member of a binary system. Our target, the nitrogen-type star WR 110 (= HD 165688) was…

天体物理学 · 物理学 2009-11-07 S. L. Skinner , S. A. Zhekov , M. Guedel , W. Schmutz

We present a VLT/FORS1 survey of Wolf-Rayet (WR) stars in the spiral galaxy NGC 1313. In total, 94 WR candidate sources have been identified from narrow-band imaging. Of these, 82 have been spectroscopically observed, for which WR emission…

天体物理学 · 物理学 2009-11-13 L. J. Hadfield , P. A. Crowther
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