C H A N D R A
S C I E N C E
C E N T E R O B S E R V A T I O N C A T A L O G |
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Abstract: The population of massive black holes (BHs) in present day low-mass galaxies is an important constraint for models of black hole formation and growth. However, these systems are generally difficult to find. We have recently identified a population of low-mass galaxies (Mstar=5x10^7 - 5x10^9 Msun) with long-term optical photometric variability consistent with an active galactic nucleus (AGN). These systems tend to lack optical spectroscopic AGN signatures, indicating they may be AGN missed by standard selection techniques. We propose joint Chandra and HST observations of 9 nearby (z<0.02) low-mass galaxies with AGN-like variability to validate this selection technique, study accretion properties, and characterize host galaxies. |
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