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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.

(a)

Classification in this paper.

(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).

(d)

Source map is contaminated by emission from other nearby sources.

(e)

Emission is extended and associated with the target source.

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