The infrared variability of the eruptive variable HM Sagittae

Details The infrared variability of the eruptive variable HM Sagittae The infrared variability of the eruptive variable HM Sagittae

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978a%26a....70l..75s&link_type=abstract

Astronomy and Astrophysics, vol. 70, no. 6, Dec. 1978, p. L75, L76.

Astronomy and Astrophysics

Astronomy

13

Binary Stars, Infrared Astronomy, Variable Stars, Periodic Variations, Stellar Models, Visual Observation

Scientific paper

Recent near infrared observations have been obtained of the peculiar eruptive variable HM Sagittae which show a general decrease in the flux levels between 1 and 5 microns during 1977-1978. The existing data are yet too sparse to ascertain the nature of the variability; however, both the IR and visual observations confirm the close resemblance of HM Sge to V1016 Cyg. A model of a binary symbiotic system containing a late type variable may be consistent with the current data.

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