H 0323+022 : a puzzling high-latitude X-ray/optical/radio source.
Abstract
A flaring X-ray source, H0323+022, has been located at high galactic latitude (b = -42°) with the scanning modulation collimator on HEAO 1 and identified with a V = 16.5 ultraviolet-excess object. The counterpart has been observed on two occasions to have zero redshift absorption lines characteristic of an F or G star in the range 3800-7300 Å, but on at least five other occasions, these features have been absent. The object also has a large infrared flux indicating a multicomponent source. Observations with the Einstein Observatory indicate that the X-ray source has two components, a steady, soft component and a variable, hard component which exhibited a pronounced 60 s dip as well as flaring activity on time scales down to 6 hours. The source has also been detected at 5 GHz with a flux density of 41 ± 1 mJy by Feigelson, Giommi, and Maccacaro.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- January 1983
- DOI:
- Bibcode:
- 1983ApJ...264L..43D
- Keywords:
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- Radio Sources (Astronomy);
- Spaceborne Astronomy;
- Ubv Spectra;
- Visible Spectrum;
- X Ray Sources;
- Absorption Spectra;
- Collimators;
- Heao 1;
- Infrared Astronomy;
- Radiant Flux Density;
- Stellar Spectrophotometry;
- Ultraviolet Astronomy;
- Astrophysics