Elemental abundance analyses with DAO spectrograms - XX. The early A stars epsilon Serpentis, 29 Vulpeculae and sigma Aquarii

Details Elemental abundance analyses with DAO spectrograms - XX. The early A stars epsilon Serpentis, 29 Vulpeculae and sigma Aquarii Elemental abundance analyses with DAO spectrograms - XX. The early A stars epsilon Serpentis, 29 Vulpeculae and sigma Aquarii

Oct 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.300..359a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 300, Issue 2, pp. 359-372.

Astronomy and Astrophysics

Astronomy

12

Stars: Abundances, Stars: Individual: Epsilon Ser, Stars: Individual: 29 Vul, Stars: Individual: Sigma Aqr

Scientific paper

Elemental abundances of the early A stars epsilon Ser, 29 Vul and sigma Aqr are derived consistently with previous studies of this series using spectrograms obtained with Reticon and CCD detectors. The derived abundances confirm that epsilon Ser is a definite Am star. 29 Vul shows evidence for a weakly operating Am star phenomenon. sigma Aqr, a hot Am star prototype, has abundances similar to those of o Peg, another class prototype.

Affiliated with

Also associated with

No associations

Rating

Elemental abundance analyses with DAO spectrograms - XX. The early A stars epsilon Serpentis, 29 Vulpeculae and sigma Aquarii 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 Elemental abundance analyses with DAO spectrograms - XX. The early A stars epsilon Serpentis, 29 Vulpeculae and sigma Aquarii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elemental abundance analyses with DAO spectrograms - XX. The early A stars epsilon Serpentis, 29 Vulpeculae and sigma Aquarii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1098891