LDN 55 , the SIMBAD biblio

LDN 55 , the SIMBAD biblio (14 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:48:08


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Title First 3 Authors
1927Barn..C......0B viz 355 ~ A photographic Atlas of selected regions of the Milky Way. BARNARD E.E.
1962ApJS....7....1L viz 1829 890 Catalogue of dark nebulae. LYNDS B.T.
1988MNRAS.235..139P 150 36 IRAS associations with dark clouds of opacity class 6. PARKER N.D.
1995ApJ...454..217W 40 52 Collapse candidates among the Bok globules. WANG Y., EVANS II N.J., ZHOU S., et al.
1997A&A...326..329L 123 126 Millimetre dust emission from northern Bok globules. LAUNHARDT R. and HENNING T.
2001MNRAS.323..257V 46 29 A SCUBA survey of compact dark Lynds clouds. VISSER A.E., RICHER J.S. and CHANDLER C.J.
2001Natur.409..159A 20 6 367 Internal structure of a cold dark molecular cloud inferred from the extinction of background starlight. ALVES J.F., LADA C.J. and LADA E.A.
2002A&A...383..631D viz 15       D               3330 41 A catalogue of dust clouds in the Galaxy. DUTRA C.M. and BICA E.
2002AJ....124.2756V 127 100 Completion of a SCUBA survey of Lynds dark clouds and implications for low-mass star formation. VISSER A.E., RICHER J.S. and CHANDLER C.J.
2006AJ....132.1998Y 36 20 Submillimeter common-user bolometer array mapping of Spitzer c2d small clouds and cores. YOUNG C.H., BOURKE T.L., YOUNG K.E., et al.
2012A&A...547A..11N 117         O X         3 19 61 The Earliest Phases of Star formation (EPoS) observed with Herschel: the dust temperature and density distributions of B68. NIELBOCK M., LAUNHARDT R., STEINACKER J., et al.
2015NewA...40...49B 79             C       1 6 3 A theoretical model for electromagnetic characterization of a spherical dust molecular cloud equilibrium structure. BORAH B. and KARMAKAR P.K.
2018MNRAS.478..784P viz 16       D               1 417 ~ Towards a comprehensive knowledge of the star cluster population in the Small Magellanic Cloud. PIATTI A.E.
2020PASJ...72....8K 43           X         1 5 ~ Distortion of magnetic fields in Barnard 68. KANDORI R., TAMURA M., SAITO M., et al.

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