A TESS view of post-eruption variability in novae V1405 Cas, V1716 Sco, and V1674 Her
We analyzed TESS archival data of three novae after recent outbursts, searching for the orbital and white dwarf (WD) rotation period and possible variations in these periods. In V1405 Cas, we detected a period of ∼116.88 seconds, which we identified as due to the WD spin, and measured a rate of incr...
Gorde:
| Egile Nagusiak: | , , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
EDP Sciences
2026-04-01
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| Saila: | Astronomy & Astrophysics |
| Gaiak: | |
| Sarrera elektronikoa: | https://www.aanda.org/articles/aa/full_html/2026/04/aa57972-25/aa57972-25.html |
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