The identification of SS73 71 as a new symbiotic star

Details The identification of SS73 71 as a new symbiotic star The identification of SS73 71 as a new symbiotic star

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...385..900p&link_type=abstract

Astronomy and Astrophysics, v.385, p.900-903 (2002)

Astronomy and Astrophysics

Astrophysics

2

Binaries: Symbiotic, Stars: Emission Line, Be

Scientific paper

We report spectroscopic observations of a new symbiotic star. This star is located in our Galaxy in the direction of the bulge and was discovered during a southern spectroscopic survey of Hα emission line objects. The star, SS73 71, after Sanduleak & Stephenson (1973), shows characteristics of a symbiotic star: the presence of TiO bands and emission lines of ions of higher ionization such as He II4686 Å, and [O III]5007 Å. Here, we present some of the main spectroscopic features, line intensities and, whenever possible, some physical parameters. Based on observations made with the 1.52 m telescope at the European Southern Observatory (La Silla, Chile) under the agreement with the Observatório Nacional, Brazil.

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