Results 21 to 30 of about 53,625 (285)
Astrophysical jets are present in a range of environments, including young stellar objects, X-ray binaries, and active galactic nuclei, but their formation is still not fully understood.
Caroline D. Huang +5 more
doaj +1 more source
Binary Interaction Dominates the Evolution of Massive Stars [PDF]
Star Partners Stars more massive than eight times the mass of the Sun are rare and short-lived, yet they are fundamentally important because they produce all the heavy elements in the universe, such as iron, silicon, and calcium. Sana et al. (p. 444
Sana, Hugues +9 more
openaire +7 more sources
Roadmap on the theoretical work of BinaMIcS [PDF]
We review the different theoretical challenges concerning magnetism in interacting binary or multiple stars that will be studied in the BinaMIcS (Binarity and Magnetic Interactions in various classes of Stars) project during the corresponding ...
Alecian, E. +4 more
core +1 more source
Eta Carinae in the Context of the Most Massive Stars [PDF]
Eta Car, with its historical outbursts, visible ejecta and massive, variable winds, continues to challenge both observers and modelers. In just the past five years over 100 papers have been published on this fascinating object.
Damineli, Augusto, Gull, Theodore R.
core +3 more sources
Interactions of binary stars [PDF]
Close Binary Stars: Observation and Interpretation. Edited by M. J. Plavec and R. K. Ulrich. Pp.598. (Reidel: 1980.) Hardback Dfl.130, $68.50; paperback Dfl.60, $31.50.
openaire +1 more source
How unique is Plaskett's star? A search for organized magnetic fields in short period, interacting or post-interaction massive binary systems [PDF]
Amongst O-type stars with detected magnetic fields, the fast rotator in the close binary called Plaskett's star shows a variety of unusual properties.
Alecian, E. +7 more
core +3 more sources
The impact of binary-star yields on the spectra of galaxies [PDF]
One of the complexities in modelling integrated spectra of stellar populations is the effect of interacting binary stars besides Type Ia supernovae (SNeIa).
Izzard, R. G., Ocvirk, P., Sansom, A. E.
core +2 more sources
Dynamically Forming Extremely Low-mass White Dwarf Binaries in Wide Orbits
The detection of a 0.2 M _⊙ extremely low-mass white dwarf (EW) in a wide orbit ( P _orb ≈ 450 days) with a 1.1 M _⊙ main-sequence companion, KIC 8145411, challenges our current understanding of how EWs form. The traditional channel for EW formation, via
Ambreesh Khurana +2 more
doaj +1 more source
The origin of single radio pulsars
By comparing relative rates of supernovae versus formation rates of single radio pulsars, recycled pulsars, binary pulsars and X-ray binaries we put strong limits on the progenitors of radio pulsars and on the requirement of an asymmetry in the supernova.
Heuvel, Edward van den +1 more
core +4 more sources
Binary Interactions in Star Clusters [PDF]
Over the past decade, a very considerable amount of effort in stellar dynamics has gone into the study of interactions between binary systems and other stars. The asymptotic analytic results obtained by Heggie (1975) for binary-single star encounters have been largely confirmed and extended by later numerical experiments (Hills 1975, Hut and Bahcall ...
openaire +1 more source

