Two evolved close binary stars: GALEX J015054.4+310745 and the central star of the planetary nebula Hen 2-84
- As part of a survey to find close binary systems among central stars of planetary nebula, we present two newly discovered binary systems.
GALEX J015054.4+310745 is identified as the central star of the possible planetary nebula Fr 2-22. We find it to be a single-lined spectroscopic binary with an orbital period of 0.2554435(10) d.
We support the previous identification of GALEX J015054.4+310745 as an sdB star and provide physical parameters for the star from spectral modelling. We identify its undetected companion as a likely He white dwarf. Based on this information, we find it unlikely that Fr 2-22 is a true planetary nebula. In addition, the central star of the true planetary nebula Hen 2-84 is found to be a photometric variable, likely due to the irradiation of a cool companion. The system has an orbital period of 0.485645(30) d.
We discuss limits on binary parameters based on the available light-curve data.
Hen 2-84 is a strongly shaped bipolar planetary nebula, which we now add to the growing list of axially orAs part of a survey to find close binary systems among central stars of planetary nebula, we present two newly discovered binary systems.
GALEX J015054.4+310745 is identified as the central star of the possible planetary nebula Fr 2-22. We find it to be a single-lined spectroscopic binary with an orbital period of 0.2554435(10) d.
We support the previous identification of GALEX J015054.4+310745 as an sdB star and provide physical parameters for the star from spectral modelling. We identify its undetected companion as a likely He white dwarf. Based on this information, we find it unlikely that Fr 2-22 is a true planetary nebula. In addition, the central star of the true planetary nebula Hen 2-84 is found to be a photometric variable, likely due to the irradiation of a cool companion. The system has an orbital period of 0.485645(30) d.
We discuss limits on binary parameters based on the available light-curve data.
Hen 2-84 is a strongly shaped bipolar planetary nebula, which we now add to the growing list of axially or point-symmetric planetary nebulae with a close binary central star.…
| Verfasserangaben: | Todd C. Hillwig, Nicole ReindlORCiDGND, Hannah M. Rotter, Adam W. Rengstorf, Ulrich HeberORCiDGND, Andreas IrrgangORCiD |
|---|---|
| DOI: | https://doi.org/10.1093/mnras/stac226 |
| ISSN: | 0035-8711 |
| ISSN: | 1365-2966 |
| Titel des übergeordneten Werks (Englisch): | Monthly notices of the Royal Astronomical Society |
| Verlag: | Oxford Univ. Press |
| Verlagsort: | Oxford |
| Publikationstyp: | Wissenschaftlicher Artikel |
| Sprache: | Englisch |
| Datum der Erstveröffentlichung: | 29.01.2022 |
| Erscheinungsjahr: | 2022 |
| Datum der Freischaltung: | 05.04.2024 |
| Freies Schlagwort / Tag: | binaries: close; planetary nebulae: individual: Hen 2-84; stars: individual: GALEX J015054.4+310745; subdwarfs |
| Band: | 511 |
| Ausgabe: | 2 |
| Seitenanzahl: | 7 |
| Erste Seite: | 2033 |
| Letzte Seite: | 2039 |
| Fördernde Institution: | Indiana Space Grant Consortium; ESO Telescopes at the La Silla or; Paranal Observatories [177.D-3023(B), 177.D-3023(C), 177.D-3023(D),; 177.D-3023(E)]; National Development and Reform Commission |
| Organisationseinheiten: | Mathematisch-Naturwissenschaftliche Fakultät / Institut für Physik und Astronomie |
| DDC-Klassifikation: | 5 Naturwissenschaften und Mathematik / 52 Astronomie / 520 Astronomie und zugeordnete Wissenschaften |
| Peer Review: | Referiert |
| Lizenz (Deutsch): |  Keine öffentliche Lizenz: Unter Urheberrechtsschutz |
