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A catalogue of symbiotic stars

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arxiv astro-ph/0005547 v1 pith:S2WDKJ2U submitted 2000-05-27 astro-ph

K.Belczynski , J.Mikolajewska , U.Munari , R.J.Ivison , M.Friedjung This is my paper · ORCID
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We present a new catalogue of symbiotic stars. In our list we include 188 symbiotic stars as well as 28 objects suspected of being symbiotic. For each star, we present basic observational material: coordinates, V and K magnitudes, ultraviolet (UV), infrared (IR), X-ray and radio observations. We also list the spectral type of the cool component, the maximum ionization potential observed, references to finding charts, spectra, classifications and recent papers discussing the physical parameters and nature of each object. Moreover, we present the orbital photometric ephemerides and orbital elements of known symbiotic binaries, pulsational periods for symbiotic Miras, Hipparcos parallaxes and information about outbursts and flickering.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Hot water emission during an outburst on a classical T Tauri star

    astro-ph.SR 2026-08 conditional novelty 7.0 of 10

    V557 Mon, a classical T Tauri star, underwent a year-long EXor outburst during which transient hot water vapor emission traced an inner disk cooling from about 3000 K to 2000 K.

  2. eRASSU J043115.8-711730: The first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    J0431-71 is a new super-soft X-ray symbiotic binary in the Magellanic Bridge whose ~524-day optical pulsation appears to drive variable accretion onto a white dwarf.

  3. High-Resolution Spectroscopy of Raman-scattered He II Lines in the Symbiotic Nova RR Telescopii

    astro-ph.SR 2026-06 unverdicted novelty 5.0 of 10

    Observations of Raman-scattered He II lines in RR Telescopii reveal distinct velocities tracing different H I depths and temporal declines in conversion efficiency, implying the neutral region needs complex radiative ...

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