ups Her, phi Her & HR 7018 abundances (Adelman+, 2001)

Details ups Her, phi Her & HR 7018 abundances (Adelman+, 2001) ups Her, phi Her & HR 7018 abundances (Adelman+, 2001)

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ycat..33670597a&link_type=abstract

VizieR On-line Data Catalog: J/A+A/367/597. Originally published in: 2001A&A...367..597A

Other

Stars: Peculiar, Abundances: Peculiar, Equivalent Widths

Scientific paper

Elemental abundances analyses are performed for the Mercury-Manganese stars υ Her, φ Her, and HR 7018 consistent with previous studies of this series using spectrograms obtained with Reticon and CCD detectors. Comparisons of the first two analyses with those performed using coadded photographic plates show the general consistency of the derived elemental abundances. For υ Her and for φ Her, abundances were newly found for O, and for Al, V, Zn, and Ce, respectively. HR 7018 is discovered to be a single-lined spectroscopic binary. Its Sc abundance is the smallest of any class member with derived abundances and its Sr abundance the largest of any known HgMn star. A correlation analysis of the most complete abundance sets for 20 HgMn stars shows that the abundances of some elements are correlated with one another and some are functions of the stellar effective temperature.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

ups Her, phi Her & HR 7018 abundances (Adelman+, 2001) 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 ups Her, phi Her & HR 7018 abundances (Adelman+, 2001), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ups Her, phi Her & HR 7018 abundances (Adelman+, 2001) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-906265