Details on Acronym: [WPK2016]
[WPK2016] (Ward-Thompson+Pattle+Kirk+, 2016) Write:<<[WPK2016] SNN>>
<<[WPK2016] HNNN>>
<<[WPK2016] FNNN>>
<<[WPK2016] NNN>> N: 25+208+138+42 Object:Core (SIMBAD class: denseCore = Dense Core) Note:JCMT SCUBA-2 850µm and Herschel SPIRE 250µm observations of the L1495 filament in the Taurus Molecular Cloud. in source:NAME Taurus Cloud Ref:=2016MNRAS.463.1008W byWARD-THOMPSON D. , PATTLE K., KIRK J.M., MARSH K., BUCKLE J., HATCHELL J., NUTTER D.J., GRIFFIN M.J., DI FRANCESCO J., ANDRE P., BEAULIEU S., BERRY D., BROEKHOVEN-FIENE H., CURRIE M., FICH M., JENNESS T., JOHNSTONE D., KIRK H., MOTTRAM J., PINEDA J., QUINN C., SADAVOY S., SALJI C., TISI S., WALKER-SMITH S., WHITE G., HILL T., KONYVES V., PALMEIRIM P., PEZZUTO S. Mon. Not. R. Astron. Soc., 463, 1008-1025 (2016) The JCMT and Herschel Gould Belt Surveys: a comparison of SCUBA-2 and Herschel data of dense cores in the Taurus dark cloud L1495. oTable 1: <[WPK2016] SNN> (Nos S1-S25). Table A1: <[WPK2016] HNNN> (Nos H1-H208). Table A2: <[WPK2016] FNNN> (Nos F1-F138). Table B1: <[WPK2016] NNN> (Nos N1-N42). =E=Catalogue in electronic form as <J/MNRAS/463/1008/> Originof the Acronym: S = Created by Simbad, the CDS Database
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