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Table 2

Spectral line properties of the HCNH+ (3–2) transition observed toward the selected positions in Serpens South.

Name αJ2000 (h m s) δJ2000 (° ′ ″) Tp (mK) υlsr (km s−1) Δυ (km s−1) Class Other names
(1) (2) (3) (4) (5) (6) (7) (8)
KAM280 18:29:57.50 −01:58:43.7 485 ± 33 7.57 ± 0.01 0.47 ± 0.02 Prestellar SerS-MM9
KAM281 18:29:57.72 −01:57:58.2 245 ± 30 7.55 ± 0.01 0.58 ± 0.03 Prestellar SerpS-MM8
KAM283 18:29:58.20 −02:01:15.2 52±18 7.55 ± 0.01 1.49 ± 0.34 Prestellar
KAM284 18:29:58.66 −02:08:22.5 <67 Prestellar
KAM289 18:30:00.85 −02:06:57.3 <56 Protostellar SerpS-MM11
KAM292 18:30:01.50 −02:10:25.5 <56 Protostellar SerpS-MM13, IRAS 18274-0212
KAM293 18:30:02.13 −02:08:15.1 <55 Prestellar SerS-MM14
KAM294 18:30:02.77 −02:01:03.4 79 ± 25 7.28 ± 0.06 1.15 ± 0.12 Prestellar SerS-MM15
KAM299 18:30:04.19 −02:03:05.5 39±5 7.49 ± 0.05 1.16 ± 0.11 Protostellar SERS 02, SerpS-MM18
KAM309 18:30:07.24 −02:12:13.6 84±10 6.25 ± 0.04 0.44± 0.09 Prestellar
KAM315 18:30:12.44 −02:06:53.6 169 ± 21 6.69 ± 0.02 0.80 ± 0.05 Protostellar SerpS-MM22

Notes. (1) Source name from Könyves et al. (2015). (2) Right ascension. (3) Declination. (4) Peak main beam brightness temperature. (5) Velocity centroid. (6) FWHM line width. (7) Classification from Könyves et al. (2015). (8) Other names from Maury et al. (2011) and Mottram et al. (2017).

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