The stellar content of low redshift BL Lac host galaxies from multicolour imaging




Hyvönen T, Kotilainen JK, Falomo R, Pursimo T

The Nuclear Region, Host Galaxy and Environment of Active Galaxies

2008

NUCLEAR REGION, HOST GALAXY AND ENVIRONMENT OF ACTIVE GALAXIES

REV MEX AST ASTR

Revista Mexicana de Astronomia y Astrofisica Serie de Conferencias

32

161

163

2

978-970-32-5297-8

1405-2059

http://www.astroscu.unam.mx/~rmaa/rmsc32_frameset.html



We present UBV-band imaging of 18 low redshift (z <= 0.3) BL Lac objects. These data are used to investigate the blue-red-near-infrared colours and colour gradients of the host galaxies. The distributions of the integrated blue/near-infrared colour and colour gradient of the BL Lac hosts are much wider than those for inactive ellipticals, and most BL Lac objects have bluer hosts and/or steeper colour gradients than those in inactive ellipticals. The blue colours are likely caused by a young stellar population component, and indicates a link between star formation caused by an interaction/merging event and the onset of the nuclear activity. This result is supported by stellar population modelling, indicating a presence of young/intermediate age populations in the majority of the sample.



Last updated on 2024-26-11 at 18:24