NOAO >   Observing Info >   Approved Programs >   2012A-0185

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Proposal Information for 2012A-0185


PI: Maria T Patterson, New Mexico State University, mtpatter@nmsu.edu
Address: Astronomy Department, 1320 Frenger Mall, P.O. Box 30001 MSC 4500, Las Cruces, NM 88003, United States

CoI: Rene Walterbos, New Mexico State University
CoI: David Thilker, Johns Hopkins University
CoI: George Heald, ASTRON
CoI: Gyula Jozsa, ASTRON
CoI: the HALOGAS team, various

Title: Continuing Observations of Stellar Streams and Star Formation in the Outskirts of HALOGAS Spiral Galaxies

Abstract: We propose to continue deep, wide-field observations in U,B, and H(alpha) of nearby spiral galaxies to map stellar streams and outer disk star forming regions, completing our observations of the HALOGAS sample. Our WSRT HALOGAS survey is studying HI gas accretion and halo gas in an unbiased sample of spiral galaxies to unprecedented sensitivity. Our goal is to understand the connection between past mergers and current gas accretion and to search for current star formation that may enrich accreting gas. We have new deep INT WFC r’ band images that show stellar halos and streams extending in some cases as far as the HI. However, we need color information to characterize their stellar populations. We also need deep, high-resolution data in a blue band to determine ages, luminosities, and masses of recently formed stars in the outer disks and halos that GALEX sees. The KPNO 4-m mosaic images will provide the depth and wide-field necessary to study faint stellar populations in extended HI halo gas and better understand the sources of accreting gas.


National Optical Astronomy Observatory, 950 North Cherry Avenue, P.O. Box 26732, Tucson, Arizona 85726, Phone: (520) 318-8000, Fax: (520) 318-8360



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