Host galaxy and spectral variability of the BL Lacertae object H0414 + 00

Details Host galaxy and spectral variability of the BL Lacertae object H0414 + 00 Host galaxy and spectral variability of the BL Lacertae object H0414 + 00

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....102.1294f&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 102, Oct. 1991, p. 1294-1297.

Astronomy and Astrophysics

Astronomy

11

Bl Lacertae Objects, Elliptical Galaxies, Galactic Clusters, H Lines, Infrared Spectra, X Ray Sources

Scientific paper

Surface photometry of the nebulosity surrounding the X-ray selected BL Lacertae object H0414 + 00 is presented. The radial profile is consistent with a giant elliptical galaxy of Mv = -23.2. Simultaneous optical to IR observations at three different epochs show wavelength-dependent variability. The spectral flux distribution is interpreted in terms of a galaxian contribution superposed onto a flat variable nonthermal component.

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