Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-04-12
Ap. J. Vol. 522, p. 424 (1999)
Astronomy and Astrophysics
Astrophysics
27 pp. + 10 figs., or offprint mailed by request to harris@tgrs2.gsfc.nasa.gov
Scientific paper
10.1086/307625
The Transient Gamma Ray Spectrometer (TGRS) on board the WIND spacecraft has spent most of the interval 1995-1997 in a high-altitude orbit where gamma-ray backgrounds are low. Its high-resolution Ge spectrometer is thus able to detect weak lines which are slightly offset from stronger background features. One such line is predicted from nucleosynthesis in classical novae, where beta-decays on a time-scale of a few hours in an expanding envelope produce positrons that annihilate to generate a line which is blueshifted by a few keV away from the background annihilation line at 511 keV. The broad TGRS field of view contained five known Galactic novae during 1995 January - 1997 June, and we have searched the spectra taken around the times of these events for the blueshifted nova annihilation line. Although no definite detections were made, the method is shown to be sensitive enough to detect novae occurring on ONeMg-rich white dwarfs out to about 2.5 kpc.
Cline Thomas L.
Gehrels Neil
Harris Mark J.
Naya Juan E.
Palmer David M.
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