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Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer
by
Kochkina, V. Yu
, Sosnovskij, A. A.
, Antonyuk, K. A.
, Pit’, N. V.
, Borisov, N. V.
, Galimova, E. K.
, Antonyuk, O. I.
, Pavlenko, E. P.
, Kolbin, A. I.
, Shugarov, S. Yu
, Spiridonova, O. I.
, Burenkov, A. N.
, Suslikov, M. V.
, Vinokurov, A. S.
in
Accretion disks
/ Astronomy
/ Astrophysics and Astroparticles
/ Cosmic rays
/ Cyclotrons
/ Eclipses
/ Emission lines
/ Light
/ Magnetic fields
/ Modelling
/ Observations and Techniques
/ Observatories
/ Orbits
/ Physics
/ Physics and Astronomy
/ Radial velocity
/ Software
/ Spectral energy distribution
/ Spectrum analysis
/ Telescopes
/ White dwarf stars
2024
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Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer
by
Kochkina, V. Yu
, Sosnovskij, A. A.
, Antonyuk, K. A.
, Pit’, N. V.
, Borisov, N. V.
, Galimova, E. K.
, Antonyuk, O. I.
, Pavlenko, E. P.
, Kolbin, A. I.
, Shugarov, S. Yu
, Spiridonova, O. I.
, Burenkov, A. N.
, Suslikov, M. V.
, Vinokurov, A. S.
in
Accretion disks
/ Astronomy
/ Astrophysics and Astroparticles
/ Cosmic rays
/ Cyclotrons
/ Eclipses
/ Emission lines
/ Light
/ Magnetic fields
/ Modelling
/ Observations and Techniques
/ Observatories
/ Orbits
/ Physics
/ Physics and Astronomy
/ Radial velocity
/ Software
/ Spectral energy distribution
/ Spectrum analysis
/ Telescopes
/ White dwarf stars
2024
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Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer
by
Kochkina, V. Yu
, Sosnovskij, A. A.
, Antonyuk, K. A.
, Pit’, N. V.
, Borisov, N. V.
, Galimova, E. K.
, Antonyuk, O. I.
, Pavlenko, E. P.
, Kolbin, A. I.
, Shugarov, S. Yu
, Spiridonova, O. I.
, Burenkov, A. N.
, Suslikov, M. V.
, Vinokurov, A. S.
in
Accretion disks
/ Astronomy
/ Astrophysics and Astroparticles
/ Cosmic rays
/ Cyclotrons
/ Eclipses
/ Emission lines
/ Light
/ Magnetic fields
/ Modelling
/ Observations and Techniques
/ Observatories
/ Orbits
/ Physics
/ Physics and Astronomy
/ Radial velocity
/ Software
/ Spectral energy distribution
/ Spectrum analysis
/ Telescopes
/ White dwarf stars
2024
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Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer
Journal Article
Spectroscopic and Photometric Study of the New Eclipsing Polar Gaia23cer
2024
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Overview
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.
Publisher
Pleiades Publishing,Springer Nature B.V
Subject
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