Abundance gradients in M31 - Comparison of results from supernova remnants and H II regions

Author:

Blair W. P.,Kirshner R. P.,Chevalier R. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 155 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. A Nitrogen-rich Supernova Remnant in M31: Interaction with the Circumstellar Medium at Late Times;The Astrophysical Journal;2023-08-28

2. High-resolution Spectra of Supernova Remnants in M83;The Astrophysical Journal;2023-01-01

3. Red Supergiants in M31 and M33. II. The Mass-loss Rate;The Astrophysical Journal;2021-05-01

4. New optically identified supernova remnants in the Large Magellanic Cloud;Monthly Notices of the Royal Astronomical Society;2020-11-02

5. Bar effect on gas-phase abundance gradients. I. Data sample and chemical abundances;Monthly Notices of the Royal Astronomical Society;2020-08-18

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