SAO 38830, a New Eclipsing Binary in Perseus

Details SAO 38830, a New Eclipsing Binary in Perseus SAO 38830, a New Eclipsing Binary in Perseus

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989javso..18....1b&link_type=abstract

The Journal of the American Association of Variable Star Observers. vol. 18, no. 1, p. 1-2

Physics

3

Sao 38830

Scientific paper

Visual observations indicate that a recently discovered eighth magnitude
variable (SAO 38830) is an eclipsing binary with a period of 3.0461 or
6.0922 days.

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