Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer
We present the results of our optical study of the eclipsing polar Gaia23cer. We analyze the orbital brightness variability in high () and low () states. The system has an orbital period min and exhibits deep eclipses with a duration s. The spectra have a red cyclotron continuum with the Zeeman H ab...
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Pleiades Publishing
2024
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ir-123456789-291702024-10-30T08:12:05Z Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer Kolbin, A. I. Колбин, А. И. AT2023row) Spectroscopy Photometry Cataclysmic variables Individual: Gaia23cer (ZTF18abunixr Novae We present the results of our optical study of the eclipsing polar Gaia23cer. We analyze the orbital brightness variability in high () and low () states. The system has an orbital period min and exhibits deep eclipses with a duration s. The spectra have a red cyclotron continuum with the Zeeman H absorption triplet forming in a magnetic field with a strength MG. The source of emission lines has a high radial velocity semi-amplitude (km s), and its eclipse lags behind the eclipse of the white dwarf. The mass and temperature K of the white dwarf have been estimated by modelling the spectral energy distribution. The eclipse duration corresponds to a donor mass and an orbital inclination. The donor temperature was estimated to be K by modelling the elliptical variability and eclipse depth. 2024-10-30T08:11:21Z 2024-10-30T08:11:21Z 2024 Статья Kolbin A.I., Pavlenko E.P., Kochkina V.Y., Vinokurov A.S., Shugarov S.Y., Sosnovskij A.A., Antonyuk K.A., Antonyuk O.I., Pit’ N.V., Suslikov M.V., Galimova E.K., Borisov N.V., Burenkov A.N., Spiridonova O.I. Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer // Astronomy Letters. - 50 (5). - pp. 335 - 349. - DOI: 10.1134/S1063773724700154 https://dspace.ncfu.ru/handle/123456789/29170 en Astronomy Letters application/pdf application/pdf Pleiades Publishing |
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English |
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AT2023row) Spectroscopy Photometry Cataclysmic variables Individual: Gaia23cer (ZTF18abunixr Novae |
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AT2023row) Spectroscopy Photometry Cataclysmic variables Individual: Gaia23cer (ZTF18abunixr Novae Kolbin, A. I. Колбин, А. И. Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer |
| description |
We present the results of our optical study of the eclipsing polar Gaia23cer. We analyze the orbital brightness variability in high () and low () states. The system has an orbital period min and exhibits deep eclipses with a duration s. The spectra have a red cyclotron continuum with the Zeeman H absorption triplet forming in a magnetic field with a strength MG. The source of emission lines has a high radial velocity semi-amplitude (km s), and its eclipse lags behind the eclipse of the white dwarf. The mass and temperature K of the white dwarf have been estimated by modelling the spectral energy distribution. The eclipse duration corresponds to a donor mass and an orbital inclination. The donor temperature was estimated to be K by modelling the elliptical variability and eclipse depth. |
| format |
Статья |
| author |
Kolbin, A. I. Колбин, А. И. |
| author_facet |
Kolbin, A. I. Колбин, А. И. |
| author_sort |
Kolbin, A. I. |
| title |
Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer |
| title_short |
Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer |
| title_full |
Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer |
| title_fullStr |
Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer |
| title_full_unstemmed |
Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer |
| title_sort |
spectroscopic and photometric study of the new eclipsing polar gaia23cer |
| publisher |
Pleiades Publishing |
| publishDate |
2024 |
| url |
https://dspace.ncfu.ru/handle/123456789/29170 |
| work_keys_str_mv |
AT kolbinai spectroscopicandphotometricstudyoftheneweclipsingpolargaia23cer AT kolbinai spectroscopicandphotometricstudyoftheneweclipsingpolargaia23cer |
| _version_ |
1842245669134270464 |