Spectroscopy of six X-ray-selected BL Lacertae candidates
Creators
- 1. Palomar Observatory, Pasadena, CA
- 2. Institute for Advanced Study, Princeton, NJ
- 3. Mount Wilson and Las Campanas Observatories, Pasadena, CA
- 4. California Univ., Irvine
- 5. Michigan Univ., Ann Arbor
- 6. Washington Univ., Seattle
Description
Results of a continuing program aimed at extending the small list of X-ray-selected BL Lac objects are reported. High-quality spectra have been obtained of six faint blue objects that lie within the positional error boxes of X-ray sources discovered serendipitously by the Einstein Observatory. Three of the objects are found to be previously uncataloged low-red-shift quasi-stellar objects, including one formerly suggested as BL Lac candidate. Two are faint galactic stars, while the final object has a featureless spectrum, and thus remains a candidate. Although X-ray selection may ultimately be an effective means of discovering faint BL Lac objects, such sources are evidently rare at the X-ray flux levels attainable by the Einstein Observatory. 15 references
Additional details
Publishing Information
- Journal Title
- Publ. Astron. Soc. Pac.
- Journal Volume
- 98
- Series
- Publ. Astron. Soc. Pac.
- Journal Page Range
- 1129-1132
- ISSN
- 0004-6280
- CODEN
- PASPA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18078110
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BL LACERTAE OBJECTS; GALAXY NUCLEI; QUASARS; SPECTRA; X RADIATION
- Descriptors DEC
- COSMIC RADIO SOURCES; COSMIC RAY SOURCES; COSMIC X-RAY SOURCES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS