Search Results - "Chene, N."
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A SYSTEMATIC SEARCH FOR COROTATING INTERACTION REGIONS IN APPARENTLY SINGLE GALACTIC WOLF-RAYET STARS. II. A GLOBAL VIEW OF THE WIND VARIABILITY
Published in The Astrophysical journal (01-08-2011)“…This study is the second part of a survey searching for large-scale spectroscopic variability in apparently single Wolf-Rayet (WR) stars. In a previous paper…”
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A massive open cluster hiding in full sight
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT Obscuration and confusion conspire to limit our knowledge of the inner Milky Way. Even at moderate distances, the identification of stellar systems…”
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Modelling variable linear polarization produced by Co-rotating Interaction Regions (CIRs) across optical recombination lines of Wolf–Rayet stars
Published in Monthly notices of the Royal Astronomical Society (01-11-2023)“…ABSTRACT Massive star winds are structured both stochastically (‘clumps’) and often coherently (Co-rotation Interaction Regions, or CIRs). Evidence for CIRs…”
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The VVV open cluster project – II. Near-infrared sequences of 37 open clusters on eight-dimensional parameter space
Published in Monthly notices of the Royal Astronomical Society (01-07-2022)“…ABSTRACT Open clusters are key coeval structures that help us understand star formation, stellar evolution and trace the physical properties of our Galaxy. In…”
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Large-scale Periodic Variability of the Wind of the Wolf-Rayet Star WR 1 (HD 4004)
Published in The Astrophysical journal (20-06-2010)“…We present the results of an intensive photometric and spectroscopic monitoring campaign of the WN4 Wolf-Rayet (WR) star WR 1 = HD 4004. Our broadband V…”
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Metallicity Variations in the Type II Globular Cluster NGC 6934
Published in The Astrophysical journal (01-06-2018)“…Abstract The Hubble Space Telescope photometric survey of Galactic globular clusters (GCs) has revealed a peculiar “chromosome map” for NGC 6934. In addition…”
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The very massive binary NGC 3603-A1
Published in Monthly notices of the Royal Astronomical Society. Letters (01-09-2008)“…Using Very Large Telescope/Spectrograph for INtegral Field Observation in the Near-Infrared (VLT/SINFONI), we have obtained repeated adaptive-optics assisted,…”
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Analysis of physical processes in eruptive YSOs with near-infrared spectra and multiwavelength light curves
Published in Monthly notices of the Royal Astronomical Society (01-06-2021)“…ABSTRACT The decade-long Vista Variables in the Via Lactea (VVV) survey has detected numerous highly variable young stellar objects (YSOs). We present a study…”
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IRAS 18153−1651: an H ii region with a possible wind bubble blown by a young main-sequence B star
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…We report the results of spectroscopic observations and numerical modelling of the Hii region IRAS 18153-1651. Our study was motivated by the discovery of an…”
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Two massive stars possibly ejected from NGC 3603 via a three-body encounter
Published in Monthly notices of the Royal Astronomical Society. Letters (21-03-2013)“…We report the discovery of a bow-shock-producing star in the vicinity of the young massive star cluster NGC 3603 using archival data of the Spitzer Space…”
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New Galactic star clusters discovered in the disc area of the VVVX survey
Published in Monthly notices of the Royal Astronomical Society (01-12-2018)Get full text
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WR 110: A Single Wolf-Rayet Star with Corotating Interaction Regions in its Wind?
Published in The Astrophysical journal (01-07-2011)“…A 30 day contiguous photometric run with the Microvariability and Oscillations of STars (MOST) satellite on the WN5-6b star WR 110 (HD 165688) reveals a…”
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The spectral variability of a sample of WC 9 stars on time-scales of days to weeks
Published in Monthly notices of the Royal Astronomical Society (11-02-2017)“…We present the results of a spectroscopic monitoring campaign of nine presumably single Wolf-Rayet (WR) stars, eight of type WC 9 and one WC 8d. We…”
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Small-scale star formation as revealed by VVVX galactic cluster candidates
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT We report a search and analysis of obscured cluster candidates in the ‘VISTA Variables in the Via Lactea eXtended (VVVX)’ ESO Public Survey area…”
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VLT/SINFONI time-resolved spectroscopy of the central, luminous, H-rich WN stars of R136
Published in Monthly notices of the Royal Astronomical Society (21-08-2009)“…Using the Very Large Telescope's Spectrograph for INtegral Field Observation in the Near-Infrared, we have obtained repeated adaptive-optics-assisted,…”
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Discovery of a new Wolf–Rayet star and a candidate star cluster in the Large Magellanic Cloud with Spitzer
Published in Monthly notices of the Royal Astronomical Society (01-08-2014)“…We report the first-ever discovery of a Wolf–Rayet (WR) star in the Large Magellanic Cloud via detection of a circular shell with the Spitzer Space Telescope…”
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Properties of massive stars in four clusters of the VVV survey
Published in New astronomy (01-05-2016)“…•We present an analysis of massive stars in four of VVV clusters.•Determination of stellar parameters and surface abundances of the stars.•Confirmation that WC…”
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Recent developments and potentialities for reducing embryo mortality in ruminants: the role of IFN-tau and other cytokines in early pregnancy
Published in Reproduction fertility and development (1997)“…This review considers the potential reduction of embryo mortality in vitro and in vivo in ruminants. Data on cytokines provided by different fields of…”
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Spectroscopic study of the short-period WN5o + O8.5V binary system WR127 (HD 186943)
Published in Monthly notices of the Royal Astronomical Society (01-02-2011)“…Combined with previous information (orbital period P= 9.5550 d and inclination ), new optical spectroscopic data lead to improved circular orbits for this WR +…”
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MOST Finds No Coherent Oscillations in the Hot Carbon-rich Wolf-Rayet Star HD 165763 (WR 111)
Published in The Astrophysical journal (20-05-2008)“…We have photometrically monitored the V = 8 mag Galactic Population I WC5 star WR 111 for 3 weeks nonstop using the MOST microsatellite. Each of the similar to…”
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