Published November 1986 | Version v1
Journal article

Spectroscopy of six X-ray-selected BL Lacertae candidates

  • 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