Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...238..111a&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 238, no. 1-2, Nov. 1990, p. 111-115.
Astronomy and Astrophysics
Astrophysics
9
Abundance, Manganese, Mercury (Metal), Metallic Stars, Stellar Composition, Charge Coupled Devices, Metallicity, Stellar Spectra
Scientific paper
Fine analyses of limited spectral regions of the mercury-manganese stars
HR 4817 and Chi Lup confirm that these stars have abundances of typical
class members. The best determined values of HR 4817 are similar to
those of 53 Tau which is an anomalous class member.
Adelman Saul J.
Davis Philip A. G.
No associations
LandOfFree
Elemental abundances of the mercury-manganese stars HR 4817 and Chi LUPI 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 abundances of the mercury-manganese stars HR 4817 and Chi LUPI, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elemental abundances of the mercury-manganese stars HR 4817 and Chi LUPI will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-838467