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A search for Symbiotic Stars in the Local Group
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The Local Group Census is a narrow- and broad-band survey of all the galaxies of the Local Group above dec = -30 deg, in progress at the 2.5m Isaac Newton telescope on La Palma. We discuss here the ability of the survey to detect symbiotic star candidates in the Local Group, by deriving detection limits in each of the narrow- and broad-band frames used in the survey, and by estimating the total number of objects expected in each galaxy. We present two diagnostic diagrams, based on the adopted photometric filters, to discriminate between symbiotic stars and other emission-line objects such as planetary nebulae.
Forward citations
Cited by 3 Pith papers
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Symbiotic star candidates in Gaia Data Release 3
A Gaia DR3 machine-learning search yields 1,674 new symbiotic star candidates, 25 with X-ray emission.
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New Symbiotic Stars from LAMOST DR10 Spectra and Multi-band Photometry
A LAMOST DR10 survey yields two new symbiotic stars plus 12 accreting-only symbiotic candidates with inferred white dwarf temperatures near 10,000 to 15,000 K.
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New Online Database of Symbiotic Variables: Catalog and Statistical Overview of Symbiotic Binaries
NODSV is a new public catalog of ~1400 symbiotic binaries with classifications into confirmed, candidate, and misidentified categories plus a statistical overview of their properties.
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