Abstract
An improved position is presented for the X-ray source H2252-033 using
the Ariel V Sky Survey Instrument, and precise positioning using the
Scanning Modulation Collimator on HEAO-1. The source is identified
optically with a 13th magnitude emission-line object, which is probably
a white dwarf binary with a well formed accretion disk, with
similarities to the dwarf novae (e.g., SS Cyg) at minimum.
Original language | English |
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Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 193 |
DOIs | |
Publication status | Published - 1 Nov 1980 |
Keywords / Materials (for Non-textual outputs)
- Binary Stars
- Stellar Mass Accretion
- Stellar Spectrophotometry
- Variable Stars
- White Dwarf Stars
- X Ray Sources
- Emission Spectra
- Heao 3
- Novae
- Position (Location)
- Sky Surveys (Astronomy)
- Stellar Magnitude