Quasars behind the disk of M31 galaxy
Aims. Our aim is to increase the limited number of quasars behind M 31, necessary for probing the chemical content of the gas and for proper motion reference, with reliable and homogeneous redshift measurements from emission lines. Methods. We carried out spectroscopic follow-up of 32 quasar candida...
Tallennettuna:
| Päätekijät: | , , , , , , , , |
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| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
EDP Sciences
2026-04-01
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| Sarja: | Astronomy & Astrophysics |
| Aiheet: | |
| Linkit: | https://www.aanda.org/articles/aa/full_html/2026/04/aa55807-25/aa55807-25.html |
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