The very soft X-ray transient H1853 + 60

Details The very soft X-ray transient H1853 + 60 The very soft X-ray transient H1853 + 60

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.290..573s&link_type=abstract

Nature, vol. 290, Apr. 16, 1981, p. 573, 574.

Other

7

Heao 1, Radiant Flux Density, Radiation Counters, X Ray Sources, Dwarf Stars, Flare Stars, Light Curve, Novae, Variable Stars

Scientific paper

The detection of a new soft X-ray transient, H1853 + 60, using data from the Low Energy Detectors (LEDs) on the HEAO 1 A-2 experiment, is reported. Although the solar flare hypothesis cannot be ruled out, the similarity between this X-ray transient's temporal and spectral characteristics and those of several other transients observed by HEAO 1 LEDs, suggest a common emission mechanism for these events. It is unlikely that more transients as strong as these will be discovered, except on an individual scan basis.

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