Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...367..677t&link_type=abstract
Astrophysical Journal, Vol.367, NO. 2/FEB, P. 677, 1991
Astronomy and Astrophysics
Astrophysics
3
Scientific paper
We report observations of the J = 3-2 transitions of ^12^CO and ^13^CO in the starburst galaxy M82. We have detected and mapped the ^12^CO J = 3-2 transition in the nuclear region at 22" resolution. The high main beam brightness temperature of the line, 6.4 K, when compared to the J = 1-0 and J = 2-1 intensities, requires a hot (T_k_ >~ 40 K), moderately optically thin gas. We place a lower limit of ~ 15 off the I_CO_/I__^13^CO_, implying that τ_32_ <~ 6 and τ_10_ < 1 for this warm component. There are ~ 10^8^ M_sun_of warm molecular gas within a radius of 360 pc of M82. The low optical depths and high densities required to excite the J = 3-2 transition may imply sheetlike or filamentary clumping. The pressure in the molecular gas is high, nT ~ 10^6^ - 10^7^ cm^-3^ K. The unusually high pressure and filamentary nature of the interstellar medium in M82 are probably related to winds and shocks originating in the starburst.
Ho Pak Tung
Martin Robert N.
Tuner J. L.
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