Dictionary of Nomenclature of Celestial Objects
(Last update: 29-Nov-2021)

Result of query: info cati HGBS$

Details on Acronym:   HGBS
   HGBS (Herschel Gould Belt survey) Write:<<HGBS JHHMMSS.s+DDMMSS>>
<<HGBS YSO JHHMMSS.s+DDMMSS>> N: 749+536+239+532+38+1844+832+833+816 Object:Dense Core + YSO  (SIMBAD class: IR = Infra-Red source) Note:The Herschel Gould Belt Survey (HGBS) is an extensive imaging survey of the densest portions of the Gould Belt with Herschel SPIRE at 250-500 and PACS at 110-170 microns down to a 5-sigma column sensitivity NH2∼1021cm–2. The target clouds span a range of physical conditions, from active, cluster-forming complexes to quiescent regions with lower star formation activity.
For more information, visit www.herschel.fr/cea/gouldbelt/en/ in source:NAME Aquila Cloud in source:LDN 1495 in source:NAME CRA MCLD in source:NAME Lupus Cloud = NAME Lupus Complex in source:NAME Orion B in source:LDN 1157 in source:LDN 1172 in source:LDN 1228 in source:LDN 1241 in source:LDN 1251 in source:NAME Serpens Cloud in source:NAME Perseus Molecular Cloud Ref:=2015A&A...584A..91K byKOENYVES V. , ANDRE Ph., MEN'SHCHIKOV A., PALMEIRIM P., ARZOUMANIAN D., SCHNEIDER N., ROY A., DIDELON P., MAURY A., SHIMAJIRI Y., DI FRANCESCO J., BONTEMPS S., PERETTO N., BENEDETTINI M., BERNARD J.-P., ELIA D., GRIFFIN M.J., HILL T., KIRK J., LADJELATE B., MARSH K., MARTIN P.G., MOTTE F., NGUYEN LUONG Q., PEZZUTO S., ROUSSEL H., RYGL K.L.J., SADAVOY S.I., SCHISANO E., SPINOGLIO L., WARD-THOMPSON D., WHITE G.J. Astron. Astrophys., 584A, 91-91 (2015) A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey. oTables A.1-A.2, col(1): <[KAM2015] NNN> (Nos 1-749) = Tables A.1-A.2, col(2): <HGBS JHHMMSS.s+DDMMSS> N=749. Ref:=2016MNRAS.459..342M byMARSH K.A. , KIRK J.M., ANDRE P., GRIFFIN M.J., KONYVES V., PALMEIRIM P., MEN'SHCHIKOV A., WARD-THOMPSON D., BENEDETTINI M., BRESNAHAN D.W., DI FRANCESCO J., ELIA D., MOTTE F., PERETTO N., PEZZUTO S., ROY A., SADAVOY S., SCHNEIDER N., SPINOGLIO L., WHITE G.J. Mon. Not. R. Astron. Soc., 459, 342-356 (2016) A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey. oTables B1-B2, col(2): <HGBS JHHMMSS.s+DDMMSS> N=536. Ref:=2018A&A...615A.125B byBRESNAHAN D. , WARD-THOMPSON D., KIRK J.M., PATTLE K., EYRES S., WHITE G.J., KONYVES V., MEN'SHCHIKOV A., ANDRE P., SCHNEIDER N., DI FRANCESCO J., ARZOUMANIAN D., BENEDETTINI M., LADJELATE B., PALMEIRIM P., BRACCO A., MOLINARI S., PEZZUTO S., SPINOGLIO L. Astron. Astrophys., 615A, 125-127 (2018) The dense cores and filamentary structure of the molecular cloud in Corona Australis: Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey. oFig.5 Regions A-F not in SIMBAD. oTables A.1-A.2, col(2): <HGBS JHHMMSS.s+DDMMSS> N=239. Ref:=2018A&A...619A..52B byBENEDETTINI M. , PEZZUTO S., SCHISANO E., ANDRE P., KONYVES V., MEN'SHCHIKOV A., LADJELATE B., DI FRANCESCO J., ELIA D., ARZOUMANIAN D., LOUVET F., PALMEIRIM P., RYGL K.L.J., SCHNEIDER N., SPINOGLIO L., WARD-THOMPSON D. Astron. Astrophys., 619A, 52-52 (2018) A catalogue of dense cores and young stellar objects in the Lupus complex based on Herschel Gould Belt Survey observations. oTables A.1-A.2: <HGBS JHHMMSS.s+DDMMSS> N=532. Table B.1: <HGBS YSO JHHMMSS.s+DDMMSS> N=38. Ref:=2020A&A...635A..34K byKONYVES V. , ANDRE P., ARZOUMANIAN D., SCHNEIDER N., MEN'SHCHIKOV A., BONTEMPS S., LADJELATE B., DIDELON P., PEZZUTO S., BENEDETTINI M., BRACCO A., DI FRANCESCO J., GOODWIN S., RYGL K.L.J., SHIMAJIRI Y., SPINOGLIO L., WARD-THOMPSON D., WHITE G.J. Astron. Astrophys., 635A, 34-34 (2020) Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey. oTables A.1-A.2: <HGBS JHHMMSS.s+DDMMSS> N=1844. Table A.1: <[KAA2020] JHHMMSS.s+DDMMSS> N=26. Ref:=2020ApJ...904..172D byDI FRANCESCO J. , KEOWN J., FALLSCHEER C., ANDRE P., LADJELATE B., KONYVES V., MEN'SHCHIKOV A., STEPHENS-WHALE S., NGUYEN-LUONG Q., MARTIN P., SADAVOY S., PEZZUTO S., FIORELLINO E., BENEDETTINI M., SCHNEIDER N., BONTEMPS S., ARZOUMANIAN D., PALMEIRIM P., KIRK J.M., WARD-THOMPSON D. Astrophys. J., 904, 172-172 (2020) Herschel Gould Belt Survey observations of dense cores in the Cepheus Flare clouds. oTables C1-C2: <HGBS JHHMMSS.s+DDMMSS> N=832. Ref:=2021MNRAS.500.4257F byFIORELLINO E. , ELIA D., ANDRE P., MEN'SHCHIKOV A., PEZZUTO S., SCHISANO E., KONYVES V., ARZOUMANIAN D., BENEDETTINI M., WARD-THOMPSON D., BRACCO A., DI FRANCESCO J., BONTEMPS S., KIRK J., MOTTE F., MOLINARI S. Mon. Not. R. Astron. Soc., 500, 4257-4276 (2021) The census of dense cores in the Serpens region from the Herschel Gould Belt Survey. oTables A1-A2: <HGBS JHHMMSS.s+DDMMSS> N=833. Ref:=2021A&A...645A..55P byPEZZUTO S. , BENEDETTINI M., DI FRANCESCO J., PALMEIRIM P., SADAVOY S., SCHISANO E., LI CAUSI G., ANDRE P., ARZOUMANIAN D., BERNARD J.-P., BONTEMPS S., ELIA D., FIORELLINO E., KIRK J.M., KONYVES V., LADJELATE B., MEN'SHCHIKOV A., MOTTE F., PICCOTTI L., SCHNEIDER N., SPINOGLIO L., WARD-THOMPSON D., WILSON C.D. Astron. Astrophys., 645A, 55-55 (2021) Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations. oTables A.1-A.3: <HGBS JHHMMSS.s+DDMMSS> N=816. Tables E.1-E.3: <[PBD2021] NNN> (Nos 1-170). oTable 5, Fig.9 HPZ regions not identified. =E=Catalogue in electronic form as <J/A+A/584/A91/> =E=Catalogue in electronic form as <J/MNRAS/459/342/> =E=Catalogue in electronic form as <J/A+A/615/A125/> =E=Catalogue in electronic form as <J/A+A/619/A52/> =E=Catalogue in electronic form as <J/A+A/635/A34/> =E=Catalogue in electronic form as <J/A+A/645/A55/> Originof the Acronym: A = Assigned by the author(s)

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