Spectroscopy of the massive interacting binary UU Cassiopeiae [PDF]
Astronomy & Astrophysics, 2022 Context. The eclipsing close binary UU Cas is an interacting massive double-periodic system with a gainer star partly hidden in an accretion disk. Aims.
P. Hadrava +11 more
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Quasiequilibrium configurations of binary systems of dark matter admixed neutron stars [PDF]
Physical Review D, 2023 Using an adapted version of the SGRID code, we construct for the first time consistent quasi-equilibrium configurations for a binary system consisting of two neutron stars in which each is admixed with dark matter.
H. Rüter +3 more
semanticscholar +1 more source
Interacting supernovae from wide massive binary systems [PDF]
Astronomy & Astrophysics, 2023 The features in the light curves and spectra of many I and II supernovae (SNe) can be understood by assuming an interaction of the SN ejecta with circumstellar matter (CSM) surrounding the progenitor star.
A. Ercolino +3 more
semanticscholar +1 more source
Astronomy & AstrophysicsThe black holes discovered using Gaia especially Gaia BH1 and BH2, have low-mass companions of solar-like metallicity in wide orbits. For standard formation channels of isolated binary evolution that include interactions, this extreme mass ratio is ...
Matthias U. Kruckow +12 more
openalex +2 more sources
Fast Radio Bursts from Interacting Binary Neutron Star Systems [PDF]
Astrophysical Journal, 2020 Recent observations of repeating fast radio bursts (FRBs) suggest that some FRBs reside in an environment consistent with that of binary neutron star (BNS) mergers. The bursting rate for repeaters could be very high and the emission site is likely from a
Bing Zhang
semanticscholar +1 more source
New insights on the massive interacting binary UU Cassiopeiae [PDF]
Astronomy & Astrophysics, 2020 We present the results of our study of the close binary UU Cassiopeiae based on previously published multiwavelength photometric and spectroscopic data.
R. Mennickent +9 more
semanticscholar +1 more source
Accretion and Intercycle Variations in the PMS Interacting Binary AK Sco [PDF]
Astrophysical Journal, 2020 There are only a handful of known short-period pre-main-sequence spectroscopic binaries with significant accretion rates (Class II sources). AK Sco stands out in this list because the system is composed of two equal mass F5 stars in a highly eccentric ...
A. I. Gómez de Castro +4 more
semanticscholar +1 more source
Adiabatic Mass Loss in Binary Stars. III. From the Base of the Red Giant Branch to the Tip of the Asymptotic Giant Branch [PDF]
Astrophysical Journal, 2020 The distinguishing feature of the evolution of close binary stars is the role played by the mass exchange between the component stars. Whether or not the mass transfer is dynamically stable is one of the essential questions in binary evolution.
H. Ge +3 more
semanticscholar +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]
, 2017 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 +2 more sources
The impact of binary-star yields on the spectra of galaxies [PDF]
, 2009 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