BROAD Ly alpha EMISSION FROM THREE NEARBY BL LACERTAE OBJECTS

作者：Stocke John T^*; Danforth Charles W; Perlman Eric S

来源：Astrophysical Journal, 2011, 732(2): 113.

DOI：10.1088/0004-637X/732/2/113

• BL Lacertae objects: general
• BL Lacertae objects: individual (Mrk 421, PKS 2005-489, Mrk 501, PKS 2155-304)
• galaxies: nuclei
• quasars: emission lines
• ultraviolet: galaxies

We present far-UV HST/COS spectra of four nearby BL Lac objects. BL Lac spectra are dominated by a smooth, power-law continuum which arises in a relativistic jet. However, the spectra are not necessarily featureless; weak, broad- and/or narrow-line emission is sometimes seen in high-quality optical spectra. We present detections of Ly alpha emission in HST/COS spectra of Mrk 421 (z = 0.030) and PKS 2005-489 (z = 0.071) as well as an archival HST/GHRS observation of Mrk 501 (z = 0.0337). Archival HST/STIS observations of PKS 2155-304 (z = 0.116) show no Ly alpha emission to a very low upper limit. Using the assumption that the broad-line region (BLR) clouds are symmetrically placed around the active galactic nucleus (AGN), we use these measured Lya emission features to constrain either the relativistic Gamma values for the ionizing continuum produced by the jet (in the ionization-bounded case) or the mass of warm gas (in the density-bounded case). While realistic G values can be obtained for all four cases, the values for Mrk 421 and PKS 2155-304 are high enough to suggest that covering factors of BLR clouds of similar to 1%-2% might be required to provide consistency with earlier values of Doppler boosting and viewing angles suggested for this class of BL Lacs. This discrepancy also exists in the case of M 87, where the amount of Doppler boosting in our direction is expected to be minimal, again suggestive of a small covering factor of BLR clouds. If, as these small covering factors might suggest, the assumptions of a density-bounded model could be more correct, then the observed Ly alpha luminosities require that BL Lac/FR 1 nuclei possess very little warm gas (10(-4) to 10(-5) M-circle dot) as suggested by Guilbert et al. If these clouds are in pressure balance with a hotter (similar to 10(6) K) gas, the BLR contains too little mass to power the AGN by accretion alone.

• 出版日期2011-5-10