Table 3
Spectral line transitions employed in the present study.
Transition | ν | HPBW | ![]() |
Reference | ||
---|---|---|---|---|---|---|
[MHz] | [′′ ] | [pc] | [′′] | [pc] | ||
o-H2D+ (11, 0 − 11, 1) | 372 421.35580 | 16.8 | 0.034 | 0 | 0 | This work |
N2H+ (4− 3) | 372 672.526 | 16.7 | 0.034 | 0 | 0 | This work |
DCO+ (5− 4) | 360 169.7771 | 17.3 | 0.035 | 0 | 0 | This work |
C18O(2− 1) | 219 560.3568 | 28.4 | 0.058 | 2.2 | 0.004 | Miettinen (2016) (b) |
C17O(2− 1) | 224 714.199 | 27.8 | 0.057 | 0 | 0 | Miettinen & Offner (2013b) (c) |
… | … | … | 6.0–18.7 | 0.012–0.038 | Miettinen et al. (2012) | |
N2D+ (3− 2) | 231 321.912 | 27.0 | 0.055 | 0 | 0 | Miettinen & Offner (2013b) (c) |
… | … | … | 6.0–18.7 | 0.012–0.038 | Miettinen et al. (2012) | |
p-NH3 (1, 1) | 23 694.4955 | 40 | 0.081 | 6.0–18.7 | 0.012–0.038 | Miettinen et al. (2010) |
p-NH3 (2, 2) | 23 722.6333 | 40 | 0.081 | 6.0–18.7 | 0.012–0.038 | Miettinen et al. (2010) |
Notes. (a) Offset with respect to the present o-H2D+ target positions. When this offset is different for different target source, a range of values is quoted (cf. Table 1). (b) The C18O(2−1) line was observed only towards SMM 3. (c)Miettinen & Offner (2013b) studied the prestellar core SMM 6 (their source SMM 6a corresponds to the present target position).
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