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HST Observations of the Host Galaxies of BL Lacertae Objects | | C. Megan Urry
; Renato Falomo
; Riccardo Scarpa
; Joseph E. Pesce
; Aldo Treves
; Mauro Giavalisco
; | | Date: |
5 Sep 1998 | | Subject: | astro-ph | | Affiliation: | 1,2), Joseph E. Pesce , Aldo Treves , Mauro Giavalisco (STScI, Univ. Padova, Penn. State Univ., Univ. Milan at Como, Carnegie Obs. | | Abstract: | Six BL Lac objects from the complete 1 Jy radio-selected sample of 34 objects were observed in Cycle 5 with the HST WFPC2 camera to an equivalent limiting flux of mu_I~26 mag/arcsec^2. Here we report results for the second half of this sample, as well as new results for the first three objects, discussed previously by Falomo et al. (1997). In addition, we have analyzed in the same way HST images of three X-ray-selected BL Lacs observed by Jannuzi et al. (1997). The ensemble of 9 BL Lac objects spans the redshift range from z=0.19 to ~1. Host galaxies are clearly detected in seven cases, while the other two, at z~0.258 (redshift highly uncertain) and z=0.997, are not resolved. The HST images constitute a homogeneous data set with unprecedented morphological information between a few tenths of an arcsecond and several arcseconds from the nucleus, allowing us in 6 of the 7 detected host galaxies to rule out definitively a pure disk light profile. The host galaxies are luminous ellipticals with an average absolute magnitude of M_I~-24.6 mag (with dispersion 0.7 mag), more than a magnitude brighter than L* and comparable to brightest cluster galaxies. The morphologies are generally smooth and have small ellipticities (epsilon<0.2). Given such roundness, there is no obvious alignment with the more linear radio structures. In the six cases for which we have HST WFPC2 images in two filters, the derived color profiles show no strong spatial gradients and are as expected for K-corrected passively evolving elliptical galaxies. The host galaxies of the radio-selected and X-ray-selected BL Lacs for this very limited sample are comparable in both morphology and luminosity. | | Source: | arXiv, astro-ph/9809060 | | Services: | Forum | Review | PDF | Favorites | |
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