Results 21 to 30 of about 18,267 (299)

Stellar mass ejections [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
AbstractIt has been known for some time now that rapidly-rotating solar-like stars possess the stellar equivalent of solar prominences. These may be three orders of magnitude more massive than their solar counterparts, and their ejection from the star may form a significant contribution to the loss of angular momentum and mass in the stellar wind.
Jardine, Moira   +2 more
openaire   +3 more sources

Mass loss and stellar superwinds [PDF]

open access: yesPhilosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2017
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 mass of the star prior to explosion and (ii) observations of the circumstellar material around SNe may teach us the type of progenitor that made the SN.
openaire   +3 more sources

Precise Stellar Mass and Mass-Luminosity Data [PDF]

open access: yesSymposium - International Astronomical Union, 1997
Recent progress in observing and data reduction methods for precise mass and mass-luminosity determinations in binary systems are briefly reviewed. The foundations appear to have been laid for a new burst of accurate data. Detailed model simulations of the individual systems are the best way to use these data to critically test the theoretical models ...
openaire   +1 more source

Mass Measurements of Stellar and Intermediate-Mass Black Holes [PDF]

open access: yesSpace Science Reviews, 2013
28 pages, 12 figures. Accepted for publication in Space Science Reviews (DOI 10.1007/s11214-013-0030-6). Also to appear in hard cover in the Space Sciences Series of ISSI "The Physics of Accretion onto Black Holes" (Springer Publisher).
Casares, J., Jonker, P.G.
openaire   +6 more sources

Mass loss at the lowest stellar masses [PDF]

open access: yesAstronomy & Astrophysics, 2005
Accepted for publication in A&A, 8 pages, 5 figures, 2 ...
Fernandez, M., Comeron, F.
openaire   +2 more sources

Low-Mass and Sub-stellar Eclipsing Binaries in Stellar Clusters [PDF]

open access: yes, 2020
30 pages, 5 figures, no table.
Lodieu, Nicolas   +2 more
openaire   +2 more sources

Topics in Core-Collapse Supernova Theory: The Formation of Black Holes and the Transport of Neutrinos [PDF]

open access: yes, 2012
Core-Collapse Supernovae are one of the most complex astrophysical systems in the universe. They deeply entwine aspects of physics and astrophysics that are rarely side by side in nature.
O'Connor, Evan Patrick
core   +1 more source

THE UNIVERSAL STELLAR MASS-STELLAR METALLICITY RELATION FOR DWARF GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2013
24 pages, 13 figures, 1 machine-readable table included in "Other formats," accepted to ApJ.
Kirby, E.V.   +5 more
openaire   +3 more sources

Stellar masses of star forming galaxies in clusters [PDF]

open access: yes, 2010
Magister Scientiae - MScWe determine the stellar mass of star forming galaxies in the X-ray luminous cluster MS 0451.6-0305 at z ∼ 0.54. The stellar masses are estimated from fitting model spectral energy distributions (SEDs) to deep, optical UBRIz ...
Randriamampandry, Solohery Mampionona
core   +1 more source

The evolution of the stellar mass versus halo mass relationship [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
We present an analysis of the predictions made by the Galform semi-analytic galaxy formation model for the evolution of the relationship between stellar mass and halo mass. We show that for the standard implementations of supernova feedback and gas reincorporation used in semi-analytic models, this relationship is predicted to evolve weakly over the ...
Mitchell, Peter D.   +3 more
openaire   +4 more sources

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