Upper limits to X-ray emission from nova Vulpeculae

Details Upper limits to X-ray emission from nova Vulpeculae Upper limits to X-ray emission from nova Vulpeculae

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977natur.267..685c&link_type=abstract

Nature, vol. 267, June 23, 1977, p. 685, 686.

Astronomy and Astrophysics

Astronomy

5

Novae, Radiant Flux Density, Stellar Radiation, X Ray Astronomy, Periodic Variations, Range (Extremes), Stellar Luminosity

Scientific paper

A search has been made through Ariel V data for times at which an optical nova was within the field of view of the Rotation Modulation Collimator (Experiment A). Ten orbits of observations in October 1976 coincided with the maximum of nova Vulpeculae which was within the field of view from October 20.83 UT to October 21.53 UT. No significant X-ray flux was detected. The upper limits to the X-ray flux from nova Vulpeculae for each orbit are listed in a table.

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