Jet-star near the sun

Details Jet-star near the sun Jet-star near the sun

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982s%26w....21..283k&link_type=abstract

Sterne und Weltraum, vol. 21, July-Aug. 1982, p. 283. In German.

Computer Science

Binary Stars, Red Giant Stars, Stellar Winds, Variable Stars, Plasma Jets, Stellar Atmospheres, Sun, White Dwarf Stars

Scientific paper

The variable red giant R Aquarii has a period of about a year, a magnitude between six and eleven, is 750 light-years distant from the sun, and emits a jet travelling at 2000 km/s. The star is believed to have a white dwarf companion which is surrounded by the red giant's outer atmosphere, forming a symbiotic star. The star may be surrounded at the equator by an accretion disk of diameter 25 A.U.

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