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相关论文: New insights into the WR nebula M1-67 with SITELLE

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In 1997 and 2008 we used the WFPC2 camera on board of the Hubble Space Telescope to obtain two sets of narrow-band H$\alpha$ images of the runaway Wolf-Rayet (WR) star WR 124 surrounded by its nebula M1-67. This two-epoch imaging provides…

太阳与恒星天体物理 · 物理学 2015-05-20 S. V. Marchenko , A. F. J. Moffat , P. A. Crowther

We present a 3D mapping of the Wolf-Rayet (WR) nebula M1-67 around WR124. We obtained high-resolution San Pedro M\'{a}rtir (SPM) Manchester Echelle Spectrograph (MES) observations along 17 long-slit positions covering all morphological…

太阳与恒星天体物理 · 物理学 2022-05-04 S. Zavala , J. A. Toalá , E. Santamarí , G. Ramos-Larios , L. Sabin , J. A. Quino-Mendoza , G. Rubio , M. A. Guerrero

A new point of view on the dynamics of the circumstellar nebula M1-67 around the run-away Wolf-Rayet (WR) star WR 124 is presented. We found that it has been interacting with the surrounding ISM and has formed a bow shock due to its high…

天体物理学 · 物理学 2009-11-07 M. V. van der Sluys , H. J. G. L. M. Lamers

This work aims to disentangle the morphological, kinematic, and chemical components of the nebula M1-67 to shed light on its process of formation around the central Wolf-Rayet (WR) star WR124. We have carried out integral field spectroscopy…

Infrared Herschel imaging and spectroscopic observations of the nebula M1-67 around the Wolf-Rayet star WR 124 have been obtained along with optical imaging observations. The infrared images reveal a clumpy dusty nebula that extends up to 1…

太阳与恒星天体物理 · 物理学 2016-03-23 C. Vamvatira-Nakou , D. Hutsemekers , P. Royer , C. Waelkens , M. A. T. Groenewegen , M. J. Barlow

We use WR124 (WN8h) and its associated nebula M1-67, to test theoretical non-LTE models for Wolf-Rayet (WR) stars. Lyman continuum ionizing flux distributions derived from a stellar analysis of WR124, are compared with nebular properties…

天体物理学 · 物理学 2007-05-23 P. A. Crowther , A. Pasquali , O. De Marco , W. Schmutz , D. J. Hillier , A. de Koter

The Wolf-Rayet nebula M1-67 around WR124 is located above the Galactic plane in a region mostly empty of interstellar medium, which makes it the perfect target to study the mass-loss episodes associated with the late stages of massive star…

太阳与恒星天体物理 · 物理学 2020-08-12 P. Jiménez-Hernández , S. J. Arthur , J. A. Toalá

We have conducted an analysis of nebulae around Wolf-Rayet (WR) stars in M33 using data collected by the imaging Fourier transform spectrometer SITELLE at the Canada-France-Hawaii telescope as part of the SIGNALS Large Program. Of the 211…

We present a morphological study of nebulae around Wolf-Rayet (WR) stars using archival narrow-band optical and Wide-field Infrared Survey Explorer (WISE) infrared images. The comparison among WISE images in different bands and optical…

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

Among different types of massive stars in advanced evolutionary stages is the enigmatic WN8h type. There are only a few Wolf-Rayet (WR) stars with this spectral type in our Galaxy. It has long been suggested that WN8h-type stars are the…

We present the first radio--continuum detection of the circumstellar shell around the well-known WN8 type Wolf-Rayet star WR16 at 943.5\,MHz using the \ac{ASKAP} \ac{EMU} survey. At this frequency, the shell has a measured flux density of…

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 present the very first wide-field, 11 by 11 arcmin, optical spectral mapping of M16, one of the most famous star-forming regions in the Galaxy. The data were acquired with the new imaging Fourier transform spectrograph SITELLE mounted on…

星系天体物理 · 物理学 2020-03-25 Nicolas Flagey , Anna F. McLeod , Laura Aguilar , Simon Prunet

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 report a multi-wavelength study of the Wolf Rayet (WR) star: [KSF2015] 1381-19L, which is located in the solar metallicity region (Z=0.014) of the Milky Way Galaxy, strongly obscured by the interstellar dust. We perform a detailed…

太阳与恒星天体物理 · 物理学 2024-06-13 Subhajit Kar , Ramkrishna Das , Tapas Baug

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 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

We present a detailed description of the wavelength, astrometric and photometric calibration plan for SITELLE, the imaging Fourier transform spectrometer attached to the Canada-France-Hawaii telescope, based on observations of a red (647 -…

星系天体物理 · 物理学 2017-12-06 Thomas B. Martin , Laurent Drissen , Anne-Laure Melchior

In a search for new Galactic planetary nebulae from our systematic scans of the Anglo-Australian Observatory/United Kingdom Schmidt Telescope (AAO/UKST) Halpha survey of the Southern Galactic Plane, we have identified a Pop I Wolf-Rayet…

天体物理学 · 物理学 2011-03-10 Martin Cohen , Quentin A. Parker , Anne J. Green

We present high spatial resolution mid-infrared images of the nebula around the late-type carbon-rich Wolf-Rayet (WC)-OB binary system WR~112 taken by the recently upgraded VLT spectrometer and imager for the mid-infrared (VISIR) with the…

太阳与恒星天体物理 · 物理学 2017-02-08 R. M. Lau , M. J. Hankins , R. Schödel , J. Sanchez-Bermudez , A. F. J. Moffat , M. E. Ressler
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