Spectroscopic atlas of o Per 3826-4882{AA} (Gulliver+, 2004)

Details Spectroscopic atlas of o Per 3826-4882{AA} (Gulliver+, 2004) Spectroscopic atlas of o Per 3826-4882{AA} (Gulliver+, 2004)

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34130285g&link_type=abstract

VizieR On-line Data Catalog: J/A+A/413/285. Originally published in: 2004A&A...413..285G

Physics

Stars: Early-Type, Spectroscopy

Scientific paper

We present a spectroscopic atlas of the sharp-lined, hot metallic-line star o Pegasi (A1 IV) based on spectrograms obtained with the long camera of the 1.22-m telescope of the Dominion Astrophysical Observatory using a Reticon detector. For 3826-4882 the inverse dispersion is 2.4{AA}/mm with a resolution of 0.072{AA}. At the continuum the mean signal-to-noise ratio is 800. The wavelengths in the laboratory frame, the equivalent widths, and the identifications of the various spectral features are given. The stellar and synthetic spectra with their corresponding line identifications can be examined at http://www.brandonu.ca/physics/gulliver/atlases.html .
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Spectroscopic atlas of o Per 3826-4882{AA} (Gulliver+, 2004) 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 Spectroscopic atlas of o Per 3826-4882{AA} (Gulliver+, 2004), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic atlas of o Per 3826-4882{AA} (Gulliver+, 2004) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-773494