Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientific paper
2009-05-28
Astron.J.137:4670,2009
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
28 pages, 34 figures, published in AJ (http://adsabs.harvard.edu/abs/2009AJ....137.4670L)
Scientific paper
10.1088/0004-6256/137/6/4670
We present the HERA CO-Line Extragalactic Survey (HERACLES), an atlas of CO emission from 18 nearby galaxies that are also part of The HI Nearby Galaxy Survey (THINGS) and the Spitzer Infrared Nearby Galaxies Survey (SINGS). We used the HERA multi-pixel receiver on the IRAM 30-m telescope to map the CO J=2-1 line over the full optical disk (defined by the isophotal radius r_25) of each target, at 13" angular resolution and 2.6 km/s velocity resolution. Here we describe the observations and reduction of the data and show channel maps, azimuthally averaged profiles, integrated intensity maps, and peak intensity maps. The implied H2 masses range from 7 \times 10^6 to 6 \times 10^9 M_sun, with four low metallicity dwarf irregular galaxies yielding only upper limits. In the cases where CO is detected, the integrated H2-to-HI ratios range from 0.02 - 1.13 and H2-to-stellar mass ratios from 0.01 to 0.25. Exponential scale lengths of the CO emission for our targets are in the range 0.8 - 3.2 kpc, or 0.2 \pm 0.05 r_25. The intensity-weighted mean velocity of CO matches that of HI very well, with a 1\sigma scatter of only 6 km/s. The CO J=2-1 / J=1-0 line ratio varies over a range similar to that found in the Milky Way and other nearby galaxies, \sim 0.6 - 1.0, with higher values found in the centers of galaxies. The typical line ratio, \sim 0.8, could be produced by optically thick gas with an excitation temperature of \sim 10 K.
Bigiel Frank
Brinks Elias
de Blok J. G. W.
Kennicutt Robert C.
Kramer Carsten
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