HR 8844: A New Transition Object between the Am Stars and the HgMn Stars?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/854/i=1/a=50/pdf
Reference60 articles.
1. Elemental abundance analyses with coadded DAO spectrograms - VI. The mercury-manganese stars Nu Cancri, Iota Coronae Borealis and HR 8349
2. Elemental abundance analyses with DAO spectrograms - VII. The late normal B stars Pi Ceti, 134 Tauri, 21 Aquilae, and Nu Capricorni and the use of Reticon spectra
3. Lifetime measurements and calculations in Y+ and Y2+ ions
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1. Non-LTE abundance analysis of A-B stars with low rotational velocities – II. Do A-B stars with normal abundances exist?;Monthly Notices of the Royal Astronomical Society;2023-09-22
2. The Surface Composition of Six Newly Discovered Chemically Peculiar Stars. Comparison to the HgMn Stars mu Lep and beta Scl and the Superficially Normal B Star nu Cap;The Astronomical Journal;2023-07-07
3. The Behavior of HgMn Stars in the Far UV—Paper 25: HD 77350;Research Notes of the AAS;2023-01-17
4. Chemically Peculiar Stars in the Open Cluster Stock 2;The Astronomical Journal;2022-11-18
5. Probable nature of HD 196821: Is the star a cool HgMn ?;Astronomische Nachrichten;2022-09-06
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