Spectrophotometry of peculiar B and A stars. XV - Alpha Andromedea, AR Aurigae, 36 Aurigae, 36 Lyncis, Phi Herculis, HR 6127, and HR 6997

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

28

A Stars, B Stars, Metallic Stars, Peculiar Stars, Stellar Spectrophotometry, Astronomical Catalogs, Continuous Spectra, Spectral Energy Distribution, Visible Spectrum

Scientific paper

Optical region energy distributions are presented for the HgMn stars α And, AR Aur, ø Her, and HR 6997; 36 Lyn and HR 6127 which may be related to the HgMn stars; and the mild Ap star 36 Aur. The possible variability of α And is examined. The observations of the binary AR Aur are fit with the aid of the parameters derived by Johansen's study of this system. The λ5200 feature is considerably stronger in 36 Lyn than in any other nonmagnetic Ap star.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Spectrophotometry of peculiar B and A stars. XV - Alpha Andromedea, AR Aurigae, 36 Aurigae, 36 Lyncis, Phi Herculis, HR 6127, and HR 6997 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 Spectrophotometry of peculiar B and A stars. XV - Alpha Andromedea, AR Aurigae, 36 Aurigae, 36 Lyncis, Phi Herculis, HR 6127, and HR 6997, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrophotometry of peculiar B and A stars. XV - Alpha Andromedea, AR Aurigae, 36 Aurigae, 36 Lyncis, Phi Herculis, HR 6127, and HR 6997 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1305345

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.