Zeeman lines and a single cyclotron line in the low-accretion rate polar 1RXS J012851.9-233931 (RBS0206)

dc.creatorSchwope, A. D.
dc.creatorSchwarz, R.
dc.creatorGreiner, J.
dc.date1999-05-31
dc.date.accessioned2026-07-07T02:31:46Z
dc.date.available2026-07-07T02:31:46Z
dc.descriptionWe present a low-resolution discovery spectrum and CCD-photometry of the bright X-ray source 1RXS J012851.9-233931 found in the ROSAT All-Sky Survey. These first observations suggest that the source is an AM Herculis star (polar) accreting at a low rate. The optical spectrum is dominated by Zeeman absorption features from the white dwarf, indicating a mean photospheric magnetic field of 36 +- 1 MG. Only weak Balmer line emission was observed. In the near infra-red, a single intense cyclotron hump was observed. The inferred magnetic field strength in the accretion plama is 45 +- 1 MG, the temperature in the plasma is below 2 keV. Likely orbital periods are ~90 min or ~146 min, the latter inside the cataclysmic variable period gap. The system is an ideal target for further detailed investigations of the field structure on a magnetic white dwarf by phase-resolved spectropolarimetry.
dc.descriptionAstron. Astrophys., in press (see also http://www.aip.de/People/ASchwope
dc.identifierhttps://arxiv.org/abs/astro-ph/9905392
dc.identifierhttp://arxiv.org/abs/astro-ph/9905392
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14272
dc.subjectAstrophysics
dc.titleZeeman lines and a single cyclotron line in the low-accretion rate polar 1RXS J012851.9-233931 (RBS0206)
dc.typetext

Files

Collections