Infrared scans of gamma ray burst source regions

Details Infrared scans of gamma ray burst source regions Infrared scans of gamma ray burst source regions

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...107l...5a&link_type=abstract

Astronomy and Astrophysics, vol. 107, no. 1, Mar. 1982, p. L5, L6.

Astronomy and Astrophysics

Astronomy

12

Dwarf Stars, Gamma Ray Bursts, Infrared Astronomy, M Stars, Neutron Stars, Radiation Sources, Astronomical Models, Radio Sources (Astronomy), Stellar Mass Accretion, Stellar Mass Ejection, Telescopes

Scientific paper

Results of infrared scans covering the error region of the gamma-ray burst event of April 6, 1979, and covering radio sources in the error region of the November 19, 1978, event are presented. No sources brighter than J = 17.5 mag were detected, and a distance exceeding 1500 pc is implied. It is suggested that the last stages of mass transfer have been detected, in which a more massive dwarf has been stripped to the lowest mass at which mass transfer can take place.

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