UVSTAR observations of Adara (epsilon CMa): 575-1250 Å

Details UVSTAR observations of Adara (epsilon CMa): 575-1250 Å UVSTAR observations of Adara (epsilon CMa): 575-1250 Å

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...383..881g&link_type=abstract

Astronomy and Astrophysics, v.383, p.881-891 (2002)

Astronomy and Astrophysics

Astrophysics

Stars: Individual: Epsilon Cma, Early-Type, Oscillations, Ultraviolet: Stars, Instrumentation: Spectrographs, Space Vehicles

Scientific paper

UVSTAR, UltraViolet Spectrograph Telescope for Astronomical Research, operates in the 500-1250 Å wave-band at 1 to 3 Å resolution. Here we report on the EUV and FUV observations of the B2 II star Adara, the brightest EUV source in the sky, obtained by UVSTAR during the STS 69 and STS 95 missions. The discussion concerns 1) wavelength and flux calibration, 2) short term time variability of selected spectral features, 3) comparison with previous measurements in the EUV band and 4) comparison with model atmospheres.

Affiliated with

Also associated with

No associations

Rating

UVSTAR observations of Adara (epsilon CMa): 575-1250 Å 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 UVSTAR observations of Adara (epsilon CMa): 575-1250 Å, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UVSTAR observations of Adara (epsilon CMa): 575-1250 Å will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1407011