Probing the Enigmatic Nuclear Source in the Dwarf Starburst Galaxy Henize 2-10 with the LBA

Computer Science

Scientific paper

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Active Galactic Nuclei / Quasars, Lba

Scientific paper

Few dwarf galaxies are known to host AGN. However, observations of these rare objects can provide important constraints on the properties of "seed" black holes that ultimately grow to millions or billions of solar masses. We propose to use the LBA to test whether the dwarf starburst galaxy Henize 2-10 harbors an obscured low-luminosity AGN (LLAGN). Previous radio continuum observations with the Very Large Array reveal a compact steep spectrum source at the dynamical center of the galaxy that is consistent with the position of a hard X-ray Chandra point source. The proposed LBA observations at 1.6 and 8.4 GHz will 1) reveal the parsec-scale structure of the radio emission, 2) determine if a large scale (~100 pc) radio jet is associated with the nuclear source, and 3) constrain the nature of the off-nuclear radio emission in Henize 2-10. The presence of a LLAGN in a dwarf starburst galaxy would greatly impact our understanding of the origin and growth of supermassive black holes and their relationship to the starburst phenomenon.

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