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Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, ISSN 1364-503X, 10/2017, Volume 375, Issue 2105, p. 20160269
Mass loss bridges the gap between massive stars and supernovae (SNe) in two major ways: (i) theoretically, it is the amount of mass lost that determines the... 
Stellar winds | Mass loss | Stellar evolution | Supernovae | stellar winds | stellar evolution | LOSS RATES | MULTIDISCIPLINARY SCIENCES | LUMINOUS BLUE VARIABLES | METALLICITY DEPENDENCE | SUPERNOVA | O-STARS | PROGENITOR | SPECTROSCOPY | RADIATION-DRIVEN WINDS | supernovae | SN 2013CU | mass loss | M-CIRCLE-DOT
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 04/2014, Volume 564
We calculate radiatively driven wind models of main-sequence B stars and provide the wind mass-loss rates and terminal velocities. The main-sequence mass-loss... 
RIGIDLY ROTATING MAGNETOSPHERE | hydrodynamics | CU VIRGINIS | stars: winds, outflows | O-STARS | HOT LUMINOUS STARS | LINE-DATA-BASE | stars: early-type | ASTRONOMY & ASTROPHYSICS | BLANKETED MODEL ATMOSPHERES | X-RAY-EMISSION | CHEMICAL-COMPOSITION | stars: mass-loss | SIGMA-ORIONIS-E | DRIVEN STELLAR WINDS
Journal Article
Annual Review of Astronomy and Astrophysics, ISSN 0066-4146, 2014, Volume 52, Issue 1, pp. 487 - 528
Our understanding of massive star evolution is in flux due to recent upheavals in our view of mass loss and observations of a high binary fraction among O-type... 
stellar winds | variables | binary stars | stellar evolution | supernovae | massive stars | EMISSION-LINE STARS | LUMINOUS BLUE VARIABLES | WOLF-RAYET STARS | O-TYPE STARS | RICH CIRCUMSTELLAR MEDIUM | BLACK-HOLE BINARIES | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | SN 2009IP CONSTRAINTS | DRIVEN STELLAR WINDS | CYGNUS OB2 ASSOCIATION | Observations | Stars | Stellar evolution
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2014, Volume 564, pp. A70 - np
We calculate radiatively driven wind models of main-sequence B stars and provide the wind mass-loss rates and terminal velocities. The main-sequence mass-loss... 
Hydrodynamics | outflows | Stars: mass-loss | Stars: winds | Stars: early-type | Stellar winds | Stellar atmospheres | B stars | Peculiar stars | Braking | Coolers | Abundance | Mathematical models | Physics - Solar and Stellar Astrophysics
Journal Article
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 06/2011, Volume 734, Issue 1, pp. 48 - jQuery1323907752442='48'
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2011, Volume 526, Issue 19, p. A162
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 11/2011, Volume 741, Issue 1, p. 54
The basic mechanisms responsible for producing winds from cool, late-type stars are still largely unknown. We take inspiration from recent progress in... 
stars: mass-loss | stars: magnetic field | stars: coronae |