Table 3
Acetone line parameters toward selected positions.
Position | RA | Dec | VLSRa | ΔVb | Trotd | Ntotd |
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Notec |
(05h35m) | (−05°22′) | (km s-1) | (km s-1) | (K) | (cm-2) | |||
|
||||||||
Ace-1 |
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7.47 ± 1.07 | 3.49 ± 1.09 | 158.7 ± 13.1 | 3.4 ± 0.1 × 1016 | 1.4 ± 0.4 × 10-8 | dM-1, MF-2, CS-3 |
Ace-2 |
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7.58 ± 1.27 | 4.46 ± 1.30 | 145.4 ± 16.2 | 2.1 ± 0.1 × 1016 | 5.5 ± 4.0 × 10-8 | CS-5, IRc7 |
Ace-3 |
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6.70 ± 1.95 | 4.20 ± 1.94 | ~100 | 6.3 ± 1.9 × 1015 | 4.8 ± 1.8 × 10-9 | MF-5, CS-6, IRc6, KL-W |
HC |
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6.87 ± 1.29 | 4.92 ± 1.37 | 141.0 ± 20.9 | 1.2 ± 0.2 × 1016 | 2.1 ± 0.4 × 10-9 | CS-1 |
Notes.Positions are given at the epoch J2000.0. Acetone column densities and fractional abundances were estimated in source sizes of 2′′ for Ace-1, Ace-2, and HC, and 17 for Ace-3.
Counterparts as observed in the deuterated methanol (dM, Peng et al. 2012), methyl formate (MF, Favre et al. 2011a), CS J = 1 − 0 (Chandler & Wood 1997), and infrared (Shuping et al. 2004; Gezari et al. 1998) emission. Note that IRc7 is offset ~1″ to the southwest from Ace-2, and IRc6 is extended.
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