Multiline CO observations of MBM 32 (Wouterloot+, 2000)

Details Multiline CO observations of MBM 32 (Wouterloot+, 2000) Multiline CO observations of MBM 32 (Wouterloot+, 2000)

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..41440123w&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/144/123. Originally published in: 2000A&AS..144..123W

Computer Science

Molecular Clouds, Carbon Monoxide

Scientific paper

Using the KOSMA 3-m telescope we have made observations of the 12CO(J=1-0), (J=2-1) and (J=3-2), and the 13CO(J=1-0) and (J=2-1) transitions of the high latitude cloud MBM 32. The backend consisted of a Medium Resolution (channel width 167kHz; MRS), or a High Resolution (channel width 38.6kHz; HRS) acousto-optical Spectrometer. The following tables contain properties of clumps derived from the maps, assuming Gaussian clump parameters from the 12CO(J=1-0) MRS data (Table 3) 12CO(J=1-0) HRS data (Table 4) 12CO(J=2-1) MRS data (Table 5) 13CO(J=1-0) HRS data (Table 6). We distinguish between different velocity components. (4 data files).

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