Wind-envelope interaction as the origin of the slow cyclic brightness variations of luminous blue variables
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N. Langer | J. Vink | A. Sander | J. Mackey | N. Grin | L. Grassitelli | G. Graefener | N. Langer
[1] A. Mahabal,et al. A Large Fraction of Hydrogen-rich Supernova Progenitors Experience Elevated Mass Loss Shortly Prior to Explosion , 2020, The Astrophysical Journal.
[2] L. Bildsten,et al. Convectively Driven 3D Turbulence in Massive Star Envelopes. I. A 1D Implementation of Diffusive Radiative Transport , 2020, The Astrophysical Journal.
[3] J. Fuller,et al. Centrifugally driven mass-loss and outbursts of massive stars , 2020, Monthly Notices of the Royal Astronomical Society.
[4] J. Black,et al. Optical and near-infrared observations of the Fried Egg Nebula , 2020, Astronomy & Astrophysics.
[5] S. Karpov,et al. Asymmetrical nebula of the M33 variable GR290 (WR/LBV) , 2020, Astronomy & Astrophysics.
[6] J. Vink,et al. Theoretical investigation of the Humphreys–Davidson limit at high and low metallicity , 2020, Astronomy & Astrophysics.
[7] J. Black,et al. Optical and near-infrared observations of the Fried Egg Nebula , 2020, Astronomy & Astrophysics.
[8] M. Kasliwal,et al. A new and unusual LBV-like outburst from a Wolf–Rayet star in the outskirts of M33 , 2020, Monthly Notices of the Royal Astronomical Society.
[9] P. Schneider,et al. Properties of OB star−black hole systems derived from detailed binary evolution models , 2019, Astronomy & Astrophysics.
[10] G. Meynet,et al. Massive Black Holes Regulated by Luminous Blue Variable Mass Loss and Magnetic Fields , 2019, The Astrophysical Journal.
[11] E. Stanway,et al. Binary population synthesis models for core-collapse gamma-ray burst progenitors , 2019, Monthly Notices of the Royal Astronomical Society.
[12] E. Pian,et al. iPTF14hls as a variable hyper-wind from a very massive star , 2019, Monthly notices of the Royal Astronomical Society.
[13] J. Vink,et al. Driving classical Wolf-Rayet winds: A Γ- and Z-dependent mass-loss , 2019, Monthly Notices of the Royal Astronomical Society.
[14] N. Kee,et al. Theoretical wind clumping predictions of OB supergiants from line-driven instability simulations across the bi-stability jump , 2019, Astronomy & Astrophysics.
[15] J. Puls,et al. New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars , 2019, Astronomy & Astrophysics.
[16] S. Ro. The Wolf–Rayet Stellar Response To The Iron Opacity Bump: Envelope Inflation, Winds, and Microturbulence , 2019, The Astrophysical Journal.
[17] E. Quataert,et al. Three Dimensional Radiation Hydrodynamic Simulations of Massive Star Envelopes , 2018, 1809.10187.
[18] E. Quataert,et al. Outbursts of luminous blue variable stars from variations in the helium opacity , 2018, Nature.
[19] J. Vink. Fast and slow winds from supergiants and luminous blue variables , 2018, Astronomy & Astrophysics.
[20] J. Vink,et al. How common is LBV S Doradus variability at low metallicity? , 2018, Astronomy & Astrophysics.
[21] R. Kotak,et al. The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst , 2018, The Astrophysical Journal.
[22] P. Crowther,et al. The luminosities of cool supergiants in the Magellanic Clouds, and the Humphreys-Davidson limit revisited , 2018, 1804.06417.
[23] N. Langer,et al. Subsonic structure and optically thick winds from Wolf–Rayet stars , 2018, Astronomy & Astrophysics.
[24] J. Groh,et al. Catching a star before explosion: the luminous blue variable progenitor of SN 2015bh , 2017, Astronomy & Astrophysics.
[25] N. Langer,et al. Metallicity dependence of envelope inflation in massive stars , 2016, 1611.07280.
[26] J. Telting,et al. The IACOB project: III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars ? , 2016, 1608.05508.
[27] J. Vink,et al. Two bi-stability jumps in theoretical wind models for massive stars and the implications for luminous blue variable supernovae , 2016, 1602.05868.
[28] N. Langer,et al. A new route towards merging massive black holes , 2016, 1601.03718.
[29] I. Mandel,et al. Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries , 2015, 1601.00007.
[30] E. Quataert,et al. LOCAL RADIATION HYDRODYNAMIC SIMULATIONS OF MASSIVE STAR ENVELOPES AT THE IRON OPACITY PEAK , 2015, 1509.05417.
[31] N. Langer,et al. OBSERVATIONAL CONSEQUENCES OF TURBULENT PRESSURE IN THE ENVELOPES OF MASSIVE STARS , 2015, 1507.03988.
[32] N. Langer,et al. Massive main sequence stars evolving at the Eddington limit , 2015, 1506.02997.
[33] N. Cox,et al. The Herschel view of the nebula around the luminous blue variable star AG Carinae , 2015, 1504.03204.
[34] D. Bizyaev,et al. New luminous blue variables in the Andromeda galaxy , 2014, 1412.5319.
[35] J. Vink,et al. On the Hα behaviour of blue supergiants: rise and fall over the bi-stability jump , 2014, 1403.4097.
[36] N. Flagey,et al. The candidate luminous blue variable G79.29+0.46: a comprehensive study of its ejecta through a multiwavelength analysis , 2014, 1402.2983.
[37] N. Smith. Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars , 2014, 1402.1237.
[38] P. Hopkins,et al. Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation , 2013, 1311.2073.
[39] Jose H. Groh,et al. Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death , 2013, 1308.4681.
[40] R. Humphreys,et al. LUMINOUS AND VARIABLE STARS IN M31 AND M33. I. THE WARM HYPERGIANTS AND POST-RED SUPERGIANT EVOLUTION , 2013, 1305.6051.
[41] G. Stinson,et al. Making Galaxies in a Cosmological Context: The Need for Early Stellar Feedback , 2012, 1208.0002.
[42] N. Langer,et al. Presupernova Evolution of Massive Single and Binary Stars , 2012, 1206.5443.
[43] M. Garcia,et al. On the nature of candidate luminous blue variables in M 33 , 2012, 1202.4409.
[44] S. Owocki,et al. Stellar envelope inflation near the Eddington limit - Implications for the radii of Wolf-Rayet stars and luminous blue variables , 2011, 1112.1910.
[45] N. Morrell,et al. WIND STRUCTURE AND LUMINOSITY VARIATIONS IN THE WOLF–RAYET/LUMINOUS BLUE VARIABLE HD 5980 , 2011 .
[46] N. Langer,et al. The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a Γ-dependence of Wolf-Rayet type mass loss , 2011, 1106.5361.
[47] J. Groh,et al. ON THE NATURE OF THE PROTOTYPE LUMINOUS BLUE VARIABLE AG CARINAE. II. WITNESSING A MASSIVE STAR EVOLVING CLOSE TO THE EDDINGTON AND BISTABILITY LIMITS , 2011, 1105.0814.
[48] C. Evans,et al. Rotating massive main-sequence stars - I. Grids of evolutionary models and isochrones , 2011, 1102.0530.
[49] N. Langer,et al. Predictions of the effect of clumping on the wind properties of O-type stars , 2011 .
[50] V. F. Polcaro,et al. OPTICAL SPECTROPHOTOMETRIC MONITORING OF THE EXTREME LUMINOUS BLUE VARIABLE STAR GR 290 (ROMANO's STAR) IN M 33 , 2011 .
[51] Alexei V. Filippenko,et al. Luminous blue variable eruptions and related transients: diversity of progenitors and outburst properties , 2010, 1010.3718.
[52] Leonid Georgiev,et al. A ∼ 40 YEAR VARIABILITY CYCLE IN THE LUMINOUS BLUE VARIABLE/WOLF–RAYET BINARY SYSTEM HD 5980? , 2010 .
[53] R. Barba,et al. BONA FIDE, STRONG-VARIABLE GALACTIC LUMINOUS BLUE VARIABLE STARS ARE FAST ROTATORS: DETECTION OF A HIGH ROTATIONAL VELOCITY IN HR CARINAE , 2009, 0909.4459.
[54] A. Gal-yam,et al. A massive hypergiant star as the progenitor of the supernova SN 2005gl , 2009, Nature.
[55] J. Puls,et al. Mass loss from hot massive stars , 2008, 0811.0487.
[56] W. Hamann,et al. Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit , 2008, 0803.0866.
[57] J. Puls,et al. Bright OB stars in the Galaxy - IV. Stellar and wind parameters of early to late B supergiants , 2007, 0711.1110.
[58] Steven N. Shore,et al. Astrophysical Hydrodynamics: An Introduction , 2007 .
[59] A. Pastorello,et al. A giant outburst two years before the core-collapse of a massive star , 2007, Nature.
[60] C. Aerts,et al. Statistical properties of a sample of periodically variable B-type supergiants. Evidence for opacity , 2006, astro-ph/0611484.
[61] R. Kotak,et al. Luminous blue variables as the progenitors of supernovae with quasi-periodic radio modulations , 2006, astro-ph/0610095.
[62] N. Langer,et al. Single star progenitors of long gamma-ray bursts - I. Model grids and redshift dependent GRB rate , 2006, astro-ph/0606637.
[63] N. Langer,et al. Are luminous and metal-rich Wolf-Rayet stars inflated? , 2006 .
[64] D. Lennon,et al. Physical parameters and wind properties of galactic early B supergiants , 2005, astro-ph/0509436.
[65] A. Levan,et al. Gamma-Ray Burst Progenitors , 2016, Space Science Reviews.
[66] J. Vink,et al. The Missing Luminous Blue Variables and the Bistability Jump , 2004, astro-ph/0407202.
[67] K. Weis. On the structure and kinematics of nebulae around LBVs and LBV candidates in the LMC , 2003, astro-ph/0306501.
[68] Chris L. Fryer,et al. How Massive Single Stars End Their Life , 2002, astro-ph/0212469.
[69] Jorick S. VinkAlex de Koter. Predictions of variable mass loss for Luminous Blue Variables , 2002, astro-ph/0207170.
[70] T. Nugis,et al. The mass-loss rates of Wolf{Rayet stars explained by optically thick radiation driven wind models , 2002 .
[71] W. Schmutz,et al. Long-term spectroscopic monitoring of the Luminous Blue Variable AG Carinae , 2001 .
[72] A. M. Genderen. S Doradus variables in the Galaxy and the Magellanic Clouds , 2001 .
[73] London,et al. Mass-loss predictions for O and B stars as a function of metallicity , 2001, astro-ph/0101509.
[74] P. Massey,et al. The Progenitor Masses of Wolf-Rayet Stars and Luminous Blue Variables Determined from Cluster Turnoffs. I. Results from 19 OB Associations in the Magellanic Clouds , 2000, astro-ph/0002233.
[75] S. Woosley,et al. Presupernova Evolution of Rotating Massive Stars. I. Numerical Method and Evolution of the Internal Stellar Structure , 1999, astro-ph/9904132.
[76] M. Ueno,et al. Core-Halo Structure of a Chemically Homogeneous Massive Star and Bending of the Zero-Age Main Sequence , 1999, astro-ph/9907154.
[77] J. Cassinelli,et al. Introduction to Stellar Winds , 1999 .
[78] D. John Hillier,et al. The Treatment of Non-LTE Line Blanketing in Spherically Expanding Outflows , 1998 .
[79] C. Jager. The yellow hypergiants , 1998 .
[80] A. Nota,et al. Luminous Blue Variables: Massive Stars in Transition , 1997 .
[81] Kris Davidson,et al. Eta carinae and its environment , 1997 .
[82] Forrest J. Rogers,et al. Updated Opal Opacities , 1996 .
[83] Henny J. G. L. M. Lamers,et al. Terminal Velocities and the Bistability of Stellar Winds , 1995 .
[84] Mark Clampin,et al. Nebulae around Luminous Blue Variables: A Unified Picture , 1995 .
[85] Kris Davidson,et al. THE LUMINOUS BLUE VARIABLES: ASTROPHYSICAL GEYSERS , 1994 .
[86] C. Leitherer,et al. Geometry and physical conditions in the stellar wind of AG Carinae , 1994 .
[87] R. Chevalier,et al. Emission from circumstellar interaction in normal Type II supernovae , 1994 .
[88] H. Lamers. Mass Loss from Luminous Blue Variables , 1989 .
[89] E. Fitzpatrick,et al. The relationship between the Eddington limit, the observed upper luminosity limit for massive stars, and the luminous blue variables , 1988 .