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A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars [PDF]

open access: yesGalaxies, 2023
Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important
Paula Esther Marchiano   +6 more
doaj   +2 more sources

The Emergence of a Neutral Wind Region in the Orbital Plane of Symbiotic Binaries during Their Outbursts

open access: yesThe Astronomical Journal, 2023
Accretion of mass onto a white dwarf (WD) in a binary system can lead to stellar explosions. If a WD accretes from stellar wind of a distant evolved giant in a symbiotic binary, it can undergo occasional outbursts in which it brightens by several ...
Augustin Skopal
doaj   +1 more source

Comprehensive Analysis of a Symbiotic Candidate V503 Her

open access: yesThe Astronomical Journal, 2023
V503 Her was previously proposed as an eclipsing symbiotic candidate based on photometric behavior and spectroscopic appearance indicating the composite optical spectrum.
Jaroslav Merc   +12 more
doaj   +1 more source

ELECTRONIC TEXTBOOK FOR AMATEUR ASTRONOMERS AND STUDENTS "Binary stars and their evolution"

open access: yesOdessa Astronomical Publications, 2017
Electronic textbook for members and supervisors of the Youth Academy of Sciences; schoolars and teachers; students of the first courses. Total volume of the printed version is 86pp. The textbook is devoted to 100-th Anniversary of Prof.
L. L. Chinarova
doaj   +1 more source

Shocks and Photoionization of the Inner 650 au Jet of the Interacting Binary Star R Aquarii from Multiwavelength Hubble Space Telescope Observations

open access: yesThe Astrophysical Journal, 2023
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

An XMM-Newton View of the Symbiotic Stars HM Sge, NQ Gem, and PU Vul

open access: yesThe Astrophysical Journal, 2023
We present the analysis of archival XMM-Newton observations of the symbiotic stars HM Sge, NQ Gem, and PU Vul. The EPIC-pn spectra hint at the presence of emission lines, which are further confirmed in the first-order RGS spectra of the three sources ...
Jesús A. Toalá   +2 more
doaj   +1 more source

Symbiotic Star T CrB as an Extreme SU UMa–type Dwarf Nova

open access: yesThe Astrophysical Journal Letters, 2023
T CrB is a symbiotic recurrent nova that exhibits quiescent and active phases between its classical nova eruptions. The statistical properties of these active phases have been poorly studied thus far. Because of that their nature remained unknown.
Krystian Iłkiewicz   +2 more
doaj   +1 more source

New Symbiotic Stars or Candidates in LAMOST Low-resolution Spectra

open access: yesThe Astrophysical Journal
Symbiotic stars are among the most important binary systems for studying binary star interactions and Type Ia supernova progenitors. Based on the unique observational characteristics of symbiotic stars—strong H I and He I emission lines, giant spectral ...
Yabing Zhao   +5 more
doaj   +1 more source

Exploring Mass Transfer Mechanisms in Symbiotic Systems

open access: yesThe Astrophysical Journal
We define two regimes of the parameter space of symbiotic systems based on the dominant mass transfer mechanism. A wide range of white dwarf (WD) mass, donor mass, and donor radius combinations are explored to determine the separation for each parameter ...
Irin Babu Vathachira   +2 more
doaj   +1 more source

New Online Database of Symbiotic Variables: Catalog and Statistical Overview of Symbiotic Binaries

open access: yesThe Astrophysical Journal Supplement Series
We present the New Online Database of Symbiotic Variables (NODSV), a comprehensive and publicly accessible catalog of known and candidate symbiotic stars in the Milky Way and nearby galaxies.
Jaroslav Merc, Rudolf Gális, Marek Wolf
doaj   +1 more source

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