Chromospheric activity in bright contact binary stars
<jats:italic>Context.</jats:italic> Studying chromospheric activity of contact binaries is an effective way of revealing the magnetic activity processes of these systems. One efficient but somewhat neglected method for this purpose is to follow the changes of the H<jats:italic>α<...
Elmentve itt :
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| Dokumentumtípus: | Cikk |
| Megjelent: |
2020
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| Sorozat: | ASTRONOMY & ASTROPHYSICS
635 |
| Tárgyszavak: | |
| doi: | 10.1051/0004-6361/201937214 |
| mtmt: | 31175564 |
| Online Access: | http://publicatio.bibl.u-szeged.hu/39090 |
| Tartalmi kivonat: | <jats:italic>Context.</jats:italic> Studying chromospheric activity of contact binaries is an effective way of revealing the magnetic activity processes of these systems. One efficient but somewhat neglected method for this purpose is to follow the changes of the H<jats:italic>α</jats:italic> line profiles via optical spectroscopy. |
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| Terjedelem/Fizikai jellemzők: | 11 |
| ISSN: | 0004-6361 |