Alpha Orionis GHRS Team Project -- Cycle 1

Details Alpha Orionis GHRS Team Project -- Cycle 1 Alpha Orionis GHRS Team Project -- Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1199c&link_type=abstract

HST Proposal ID #1199

Other

Hst Proposal Id #1199

Scientific paper

The HRS will be used to obtain high signal/noise spectra of the 1980 - 3300 A spectral region of the M2 Iab supergiant Alpha Orionis. This full wavelength region will be observed at medium resolution, while 3 selected wavelength regions will be observed in the echelle mode. Exposure times have been chosen so that both the chromospheric emission line spectrum and the photospheric continuum and absorption line spectrum will be properly exposed. These observations will be combined and published in atlas format. It is hoped that this atlas will provide a standard against which high-resolution UV observations of other late-type stars can be compared. Detailed analysis of these data are planned by various IDT members.

Affiliated with

Also associated with

No associations

Rating

Alpha Orionis GHRS Team Project -- Cycle 1 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Alpha Orionis GHRS Team Project -- Cycle 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Alpha Orionis GHRS Team Project -- Cycle 1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-862387