X-ray Observations of Novae and Interstellar Matter

Details X-ray Observations of Novae and Interstellar Matter X-ray Observations of Novae and Interstellar Matter

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...206.2808k&link_type=abstract

American Astronomical Society Meeting 206, #28.08; Bulletin of the American Astronomical Society, Vol. 37, p.470

Astronomy and Astrophysics

Astronomy

Scientific paper

During their hydrostatic hydrogen burning phase novae are strong X-ray emitters with a super-soft spectrum. X-ray halos around the pointlike-novae source caused by interstellar dust grains allow to determine properties of the interstellar dust. X-ray radiation also allows to probe the properties of circumstellar dust which forms in part of the novae in the expanding envelope. Recent results will be discussed.

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