Near Infrared Brackett Gamma Imaging and Spectroscopy of Nearby Spiral Galaxies

Details Near Infrared Brackett Gamma Imaging and Spectroscopy of Nearby Spiral Galaxies Near Infrared Brackett Gamma Imaging and Spectroscopy of Nearby Spiral Galaxies

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.7304j&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #73.04; Bulletin of the American Astronomical Society, Vol. 30, p.929

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We will present, for a small sample of galaxies, Brackett Gamma (Brgamma , lambda = 2.1650 mu m) imaging and spectroscopy. We will compare these data with other, Hα (lambda = 0.6563 mu m) and FIR (40mu m - 100mu m), data to determine whether Brgamma is a good indicator of star formation in galaxies and to determine whether FIR is powered uniquely by young stars. Our data indicate that Brgamma is a superior indicator of star formation.

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