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Table 4
Properties of Perseus sources – HCO+ 3–2, and H2O obseravations in other studies.
Object | Stagea | Stage I?b | PACS H2O?c |
|
|||
J032522.3+304513 | I | − | Y |
J032536.4+304523 | I | − | Ycd |
J032637.4+301528 | I | − | N |
J032837.1+311328 | I | − | Y |
J032900.6+311200 | I | Y | − |
J032901.6+312028 | C | − | Yee |
J032904.0+311446 | C | Y | − |
J032910.7+311820 | I | Y | Ycd |
J032917.2+312746 | I | Y | − |
J032918.2+312319 | I | Y | − |
J032923.5+313329 | I | Y | − |
J032951.8+313905 | I | Y | N |
J033121.0+304530 | I | Y | Y |
J033218.0+304946 | I | Y | N |
J033313.8+312005 | C | N | − |
J033314.4+310710 | C | Y | N |
J033320.3+310721 | C | Y | − |
J033327.3+310710 | I | Y | Y |
J034356.9+320304 | I | − | Yee |
J034443.3+320131 | I | − | Yee |
Notes.
(b)
Classification from Heiderman & Evans (2015) based on single pointing detection of HCO+ 3–2.
(c)
Detection of the H2O (212–101) 179.527μm line from Herschel PACS observations (Karska et al. 2014).
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