Optical study in the field of FY Aql/GRBS 1979 0331

Details Optical study in the field of FY Aql/GRBS 1979 0331 Optical study in the field of FY Aql/GRBS 1979 0331

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989baicz..40..261h&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 40, no. 4, Aug. 1989, p. 261-266.

Astronomy and Astrophysics

Astronomy

4

Astronomical Spectroscopy, Gamma Ray Bursts, Mira Variables, Visible Spectrum, Companion Stars, Dwarf Novae, Interstellar Extinction, Symbiotic Stars

Scientific paper

Results are presented from an optical investigation of the error box of
the gamma-ray burst source (GRBS) 1979 0331. Consideration is given to
the light changes and optical behavior of the variable FY Aql, located
inside the box. The results confirm that FY Aql is a Mira variable.

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