An X-ray emitting bubble in the CEP OB3 association

Details An X-ray emitting bubble in the CEP OB3 association An X-ray emitting bubble in the CEP OB3 association

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.202..697f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 202, Feb. 1983, p. 697-701. Research supported by the Radcliffe Trust a

Astronomy and Astrophysics

Astronomy

8

Early Stars, Hot Stars, Interstellar Gas, X Ray Astronomy, B Stars, H Ii Regions, Heao 2, High Temperature Gases, Hydrogen Ions, O Stars, Stellar Winds

Scientific paper

The authors report the discovery of a region of extended X-ray emission in the young star association Cep OB3 and its H II region S155. The X-ray luminosity of 2 × 1032 erg s-1 is probably due to a bubble of hot gas formed by the winds of the early-type stars which were not individually detected. This is the first evidence for such a bubble at X-ray wavelengths.

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