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Table 1.

Properties of the sample.

Name Cloud Distancea Class Multiplicityb Observation Phase Reference Center
B335 isolated 100 pc Class 0 Single 19h37m00.9s +07°34′09″̣6
SVS13 Perseus 235 pc Class 0/I Multiple (wide) 03h29m03.1s +31°15′52″̣0
HH797 Perseus 235 pc Class 0 Multiple 03h43m57.1s +32°03′05″̣6
L1448C Perseus 235 pc Class 0 Multiple (wide) 03h25m38.9s +30°45′14″̣9
L1448N Perseus 235 pc Class 0 Multiple (close and wide) 03h25m36.3s +30°44′05″̣4
L1448-2A Perseus 235 pc Class 0 Multiple (close and wide) 03h25m22.4s +30°45′12″̣2
IRAS03282 Perseus 235 pc Class 0 Multiple (close) 03h31m20.4s +30°45′24″̣7
NGC 1333 IRAS4A Perseus 235 pc Class 0 Multiple (close) 03h29m10.5s +31°13′31″̣0
NGC 1333 IRAS4B Perseus 235 pc Class 0 Single 03h29m12.0s +31°13′08″̣0
IRAS16293 Ophiuchus 120 pc Class 0 Multiple (wide) 16h32m22.9s −24°28′36″̣0
L1157 Cepheus 250 pc Class 0 Single 20h39m06.3s +68°02′15″̣8
CB230 Cepheus 325 pc Class 0 Binary (close) 21h17m40.0s +68°17′32″̣0

Notes.

(b)

Multiplicity derived from Launhardt (2004) for IRAS03282 and CB230, Rao et al. (2009) for IRAS16293, Palau et al. (2014) for HH797, Evans et al. (2015) for B335 and from the CALYPSO survey dust continuum maps at 220 GHz (PdBI; see http://irfu.cea.fr/Projets/Calypso/, and Maury et al. 2014) for the rest of the sources.

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