High Resolution HI Distribution Of NGC 4618 and NGC 4625

Details High Resolution HI Distribution Of NGC 4618 and NGC 4625 High Resolution HI Distribution Of NGC 4618 and NGC 4625

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21342430k&link_type=abstract

American Astronomical Society, AAS Meeting #213, #424.30; Bulletin of the American Astronomical Society, Vol. 41, p.251

Astronomy and Astrophysics

Astronomy

Scientific paper

Neutral gas, especially HI, is a tracer of galaxy evolution and the on-going interactions of galaxies. This makes HI an ideal candidate with which to observe the interacting galaxies NGC 4618 and NGC 4625 in order to map the history of their interaction and understand how the interaction influences the distribution and kinematics of the ISM in both galaxies. We present new high resolution observations of NGC 4618 and NGC 4625 obtained with the Very Large Array in its B and C configurations.

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