Far UV emission spectrum and stellar wind of Sirius A

Details Far UV emission spectrum and stellar wind of Sirius A Far UV emission spectrum and stellar wind of Sirius A

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6828v&link_type=abstract

HST Proposal ID #6828

Physics

Hst Proposal Id #6828 Hot Stars

Scientific paper

Our previous HST GHRS observations of the main sequence A1 V star Sirius A have revealed completely unexpected spectral pecularities and physical properties of that well-known star such as the presence of emission features below 1220 Angstrom and the existence of a weak stellar wind. We propose to further observe these emissions to explore their origin and the stellar wind to fill the gap in our knowledge of intermediate stars.

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