Stellar α Elements Abundance Gradient in M33

Details Stellar α Elements Abundance Gradient in M33 Stellar α Elements Abundance Gradient in M33

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.263..171m&link_type=abstract

Astrophysics and Space Science, v. 263, Issue 1/4, p. 171-174 (1998).

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

In previous papers we have published preliminary results on the stellar oxygen-abundance gradient in M33 by using B-type supergiants. In the present study, we include one new B-supergiant and derive effective temperatures and gravities for these stars. The determination of atmospheric parameters is based on analyses of silicon ionisation balance.

Affiliated with

Also associated with

No associations

Rating

Stellar α Elements Abundance Gradient in M33 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 Stellar α Elements Abundance Gradient in M33, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar α Elements Abundance Gradient in M33 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1330997