S193: another non-eclipsing SW Sex star

Bibcode
1999MNRAS.305..661M
DOI
10.1046/j.1365-8711.1999.02483.x
Martínez-Pais, I. G.; Rodríguez-Gil, P.; Casares, J.
Referencia bibliográfica

Monthly Notices of the Royal Astronomical Society, Volume 305, Issue 3, pp. 661-670.

Fecha de publicación:
5
1999
Revista
Monthly Notices of the Royal Astronomical Society
Número de autores
3
Número de autores del IAC
3
Número de citas
18
Número de citas referidas
16
Descripción
We present time-resolved optical spectroscopy of the cataclysmic variable S193. The emission lines are remarkably similar to those of V795 Her and exhibit high-velocity S-waves and complex absorptions that are modulated with the orbital period. Evidence for transient anomalous spectral features is seen during the first two nights of our run. We propose that S193 and V795 Her are non-eclipsing SW Sex stars. Finally, we show that the `disc overflow' model fails to explain the Balmer line orbital behaviour in these low-inclination systems.
Tipo
Con árbitro
Acreción
Novae

Te puede interesar

  • Con árbitro
    The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
    WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, saw first light in late 2022. WEAVE comprises a new 2-deg field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU
    Jin, Shoko et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024MNRAS.530.2688J
    Número de citas
    33
  • Con árbitro
    The double low-mass white dwarf eclipsing binary system J2102-4145 and its possible evolution
    In recent years, about 150 low-mass white dwarfs (WDs), typically with masses below 0.4 M ⊙, have been discovered. The majority of these low-mass WDs are observed in binary systems as they cannot be formed through single-star evolution within Hubble time. In this work, we present a comprehensive analysis of the double low-mass WD eclipsing binary
    Antunes Amaral, L. et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024A&A...685A...9A
    Número de citas
    0
  • Con árbitro
    Morphology and Kinematics of the Gas in M51: How Interaction with NGC 5195 Has Molded the Structure of Its Arms
    The Whirlpool Galaxy is a well-studied grand design galaxy with two major spiral arms, and a large satellite NGC 5195. The arms both show long uniform sections with perturbations ("kinks" or sharp turns) in specific regions. Comparing the two arms shows a small radial offset between the main kinked regions. We analyzed the morphology and also the
    Font, Joan et al.

    Fecha de publicación:

    5
    2024
    Bibcode
    2024ApJ...966..110F
    Número de citas
    0