J/A+AS/144/123 Multiline CO observations of MBM 32 (Wouterloot+, 2000) ================================================================================ Multiline CO observations of MBM 32 Wouterloot J.G.A., Heithausen A., Schreiber W., Winnewisser G =2000A&AS..144..123W ================================================================================ ADC_Keywords: Molecular clouds ; Carbon monoxide Keywords: ISM: clouds - ISM: individual objects: MBM32 - ISM: molecules - radio lines: ISM Description: Using the KOSMA 3-m telescope we have made observations of the ^12^CO(J=1-0), (J=2-1) and (J=3-2), and the ^13^CO(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 ^12^CO(J=1-0) MRS data (Table 3) ^12^CO(J=1-0) HRS data (Table 4) ^12^CO(J=2-1) MRS data (Table 5) ^13^CO(J=1-0) HRS data (Table 6). We distinguish between different velocity components. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 09 32 46.6 +65 51 43 MBM 32 ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 64 38 Clumps found in MBM 32 using the 12CO(J=1-0) MRS data, with TR*>0.8K, and dv'>1.0km/s table4.dat 64 31 Clumps found in MBM 32 using the 12CO(J=1-0) HRS data, with TR*>1.4K, and dv'>0.4km/s table5.dat 64 53 Clumps found in MBM 32 from 12CO(J=2-1) MRS data, with TR*>0.6K, and dv'>0.6km/s table6.dat 64 22 Clumps found in MBM 32 from 13CO(J=1-0) HRS data, with TR*>0.4K, and dv'>0.3km/s tables.tex 87 309 LaTeX version of the tables -------------------------------------------------------------------------------- Byte-by-byte Description of file: table?.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 A1 --- n_Vlsr [1-3] Vlsr interval (1) 3- 7 F5.1 arcmin oRA Right ascension offset (2) 9- 13 F5.1 arcmin oDE Declination offset (2) 15- 20 F6.2 km/s Vlsr LSR (Local Standard of Rest) velocity (3) 22- 27 F6.2 K TR*peak Peak of rms noise (T^*^_R_) 29- 34 F6.2 km/s dv line width 36- 41 F6.2 pc size Gaussian FWHM 43- 48 F6.2 solMass Mass Mass 50- 54 I5 cm-3 nH2 H2 density 56- 59 I4 solMass Massvir Virial mass 63 A1 --- Remark [+-] See Note (4) -------------------------------------------------------------------------------- Note (1): Vlsr interval is coded as follows: 1: Vlsr>2km/s 2: 02km/s. Mass in these clumps: 8.73M_{sun}_ (51.8% of 16.84M_{sun}_) for 02km/s. Mass in these clumps: 4.33M_{sun}_ (45.9% of 9.43M_{sun}_) for 02km/s. Mass in these clumps: 5.92M_{sun}_ (48.8% of 12.14M_{sun}_) for 02km/s. Mass in these clumps: 3.78M_{sun}_ (48.6% of 7.77M_{sun}_) Note (4): +: indicates clumps that are clearly visible in the original channel maps without other clumps being subtracted. -: indicates clumps that are not visible in the original channel maps -------------------------------------------------------------------------------- Acknowledgements: Jan Wouterloot ================================================================================ (End) Patricia Bauer [CDW] 11-Apr-2000