AST/RO Observations of CO J=7-6 and J=4-3 Emission toward the Galactic Center Region

Details AST/RO Observations of CO J=7-6 and J=4-3 Emission toward the Galactic Center Region AST/RO Observations of CO J=7-6 and J=4-3 Emission toward the Galactic Center Region

2002-07-26

arxiv.org/abs/astro-ph/0207586v2

Astronomy and Astrophysics

Astrophysics

20 pages, 6 figures, Appear to v580 n2 ApJ December 1, 2002 issue, uncompressed figures are available at http://cfa-www.harvar

Scientific paper

We present position-velocity strip maps of the Galactic Center region in the CO J=7-6 and J=4-3 transitions observed with the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) located at Amundsen-Scott South Pole Station. Emission from the two rotational transitions of 12^CO was mapped at b=0 deg for 3.5 deg > l > -1.5 deg, on a 1' grid with a FWHM beamsize of 58'' at 806 GHz and 105'' at 461 GHz. Previous observations of CO J=4-3 (Martin et al., in preparation) and CI (Ojha et al. 2001) emission from this region show that these lines are distributed in a manner similar to CO J=1-0 (Stark et al. 1987); the (CO J=4-3)/(CO J=1-0) line ratio map is almost featureless across the entire Galactic Center region. In contrast, the CO J=7-6 emission from the Galactic Center is strongly peaked toward the Sgr A and Sgr B molecular complexes. A Large Velocity Gradient (LVG) analysis shows that aside from the two special regions Sgr A and Sgr B, the photon-dominated regions within a few hundred parsecs of the Galactic Center are remarkably uniform in mean density and kinetic temperature at n = 2500 to 4000 cm^{-3} and T=30 to 45K. The (CO J=7-6)/(CO J=4-3) line temperature ratios near Sgr B are a factor of two higher than those observed in the nuclear region of the starburst galaxy M82 (Mao et al. 2000), while the CO(J=7-6)/CO(J=4-3) line temperature ratios around Sgr A are similar to M82. The line ratio on large scales from the Galactic Center region is an order of magnitude less than that from M82.

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