S Doradus variables in the Galaxy and the Magellanic Clouds

By A. M. Genderen. 2001

182 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Computational Mechanics

View Paper: https://www.semanticscholar.org/paper/53d510d0bd36220b7c75a7b9602efc1753af8eb7

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Citations in the corpus

Massive stars exploding in a He-rich circumstellar medium. I. Type Ibn (SN 2006jc-like) events (2008, background): “An overview of our current knowledge of LBVs can be found in Van der Genderen (2001).”
PREPARING FOR AN EXPLOSION: HYDRODYNAMIC INSTABILITIES AND TURBULENCE IN PRESUPERNOVAE (2013, background): “LBVs The LBVs are a rather diverse class, consisting of a wide range of irregular variable phenomena associated with evolved massive stars (Conti 1984; Humphreys & Davidson 1994; van Genderen 2001; Smith et al. 2004, 2011b), excluding those seen in cool supergiants.”
The global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae, and the impact on the ISM evolution (2009, background): “Zickgraf (2006) listed 15 B[e] supergiants in the LMC and Van Genderen (2001) listed 21 S Dor variables.”
Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars (2014, background): “The LBVs are a rather diverse class, consisting of a wide range of irregular variable phenomena (Clark et al. 2005, Humphreys & Davidson 1994, Smith et al. 2004, 2011a, Van Dyk & Matheson 2012, van Genderen 2001).”
The Missing Luminous Blue Variables and the Bistability Jump (2004, background): “LBVs (also called S Doradus stars or Hubble-Sandage variables) exhibit a particular kind of instability, which causes a star to brighten at optical wavelengths ( V ’ 1 2 mag) as a result of a shift in the bolometric flux from the UV to the optical (see reviews by HD94; van Genderen 2001).”
Catalog of Galactic β Cephei Stars (2005, background): “Some of the S Doradus stars or LBVs (see, e.g., van Genderen 2001), also have spectral types of or near B.”
ON THE MAXIMUM MASS OF STELLAR BLACK HOLES (2009, background): “However, it is as yet not clear how much mass (if any) is lost in LBV giant eruptions in general (e.g., van Genderen 2001).”
DISCOVERY OF PRECURSOR LUMINOUS BLUE VARIABLE OUTBURSTS IN TWO RECENT OPTICAL TRANSIENTS: THE FITFULLY VARIABLE MISSING LINKS UGC 2773-OT AND SN 2009ip (2009, background): “In any case, LBVs exhibit a wide variety in ∆MV and ∆t, but a few to 10 yr is a typical observed timescale for these S Dor variations (see Humphreys & Davidson 1994; van Genderen 2001).”
Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death (2013, background): “13 that LBVs are distributed over a range of luminosities (see also van Genderen 2001; Smith et al. 2004; Clark et al. 2005, 2009a, 2012b; Vink 2012).”
Ancient eruptions of η Carinae: a tale written in proper motions (2016, background): “In its current quiescent state,η Car is substantially more luminous than most other known LBVs (e.g.,van Genderen 2001; Smith & Tombleson 2015).”
Luminous blue variables are antisocial: their isolation implies that they are kicked mass gainers in binary evolution (2014, background): “Over a dozen true LBVs are now identified in the Milky Way (MW) and the Large and Small Magellanic Clouds (LMC/SMC), and a similar number resides in other Local Group galaxies (Humphreys & Davidson 1994; van Genderen 2001; Smith et al. 2004; Clark et al. 2005).”