NAME Thumbprint Nebula , the SIMBAD biblio

NAME Thumbprint Nebula , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST18:16:17


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Title First 3 Authors
1976ApJ...208..709F 74 T                   2 63 Surface brightness profiles of dark nebulae - The
Thumbprint Nebula in Chamaeleon.
FITZGERALD M.P., STEPHENS T.C. and WITT A.N.
1995A&A...295..487L 71 T                   6 16 The Thumbprint nebula: the distribution of molecular gas and dust in a regular Bok globule. LEHTINEN K., MATTILA K., SCHNUR G.F.O., et al.
1995MNRAS.276.1052B 260 86 Studies of star formation in isolated small dark clouds - I. A catalogue of southern Bok globules : optical and IRAS properties. BOURKE T.L., HYLAND A.R. and ROBINSON G.
1996A&A...309..570L 109 T K                 7 54 Near-infrared surface brightness observations of the
Thumbprint Nebula and determination of the albedo of interstellar grains.
LEHTINEN K. and MATTILA K.
1996MNRAS.280..616J 4 9 The use of Positive Matrix Factorization in the analysis of molecular line spectra. JUVELA M., LEHTINEN K. and PAATERO P.
1997ApJ...482..796N 27 2 164 The dynamics of low-mass molecular clouds in external radiation fields. NELSON R.P. and LANGER W.D.
1997AGAb...13..128M 5 0 ISOPHOT observations of nearby molecular clouds. MATTILA K., LEMKE D., LEHTINEN K., et al.
1998A&A...333..702L 46   K                 1 31 Far-infrared ISOPHOT observations and the energy balance of a quiescent globule. LEHTINEN K., LEMKE D., MATTILA K., et al.
1999A&AS..134..241P viz 124 34 Rotation in molecular clouds. PHILLIPS J.P.
2002A&A...389..577G 12 10 The threaded molecular clumps of Chamaeleon III. GAHM G.F., LEHTINEN K., CARLQVIST P., et al.
2005A&A...437..159L 27 8 A cold globule with a Class 0/I embedded source. ISO observations of the dark cloud DC 303.8-14.2. LEHTINEN K., MATTILA K. and LEMKE D.
2005MNRAS.356..810R 10 11 ISO observations of 3-200 µm emission by three dust populations in an isolated local translucent cloud. RAWLINGS M.G., JUVELA M., MATTILA K., et al.
2005MNRAS.360..901D 23 16 New insights into the dust properties of the Taurus molecular cloud TMC-2 and its surroundings. DEL BURGO C. and LAUREIJS R.J.
2007A&A...463.1029K 112 T K     O           13 8 A comparison of density structures of a star forming and a non-star-forming globule DCld 303.8-14.2 and
Thumbprint Nebula.
KAINULAINEN J., LEHTINEN K., VAEISAENEN P., et al.
2007A&A...466..969L 15       D   O           1 21 19 ISO far-infrared observations of the high-latitude cloud L 1642. II. Correlated variations of far-infrared emissivity and temperature of ``classical large'' dust particles. LEHTINEN K., JUVELA M., MATTILA K., et al.
2008ApJS..176..164F 39           X         1 4 15 The spectral energy distribution of self-gravitating interstellar clouds. I. Spheres. FISCHERA J. and DOPITA M.A.
2009ApJ...703.1444R 38           X         1 72 7 A two micron all sky survey analysis of the stability of southern Bok globules. RACCA G.A., VILAS-BOAS J.W.S. and DE LA REZA R.
2010ApJ...710..207H 92       D     X         3 14 6 The evolution of density structure of starless and protostellar cores. HUNG C.-L., LAI S.-P. and YAN C.-H.
2013A&A...549A..91L 3042     A D     X C       78 10 4 Spectroscopy of diffuse light in dust clouds. Scattered light and the solar neighbourhood radiation field. LEHTINEN K. and MATTILA K.
2013A&A...555A.140S 39           X         1 12 19 Determination of the far-infrared dust opacity in a prestellar core. SUUTARINEN A., HAIKALA L.K., HARJU J., et al.
2014A&A...563A.106S 39           X         1 13 11 Detecting scattered light from low-mass molecular cores at 3.6 µm. Impact of global effects on the observation of coreshine. STEINACKER J., ANDERSEN M., THI W.-F., et al.
2017A&A...605A..99T viz 41           X         1 15 2 Dust properties of the cometary globule Barnard 207 (LDN 1489). TOGI A., WITT A.N. and JOHN D.S.
2023MNRAS.524.2797M 19       D               1 26 ~ Light and colour of cirrus, translucent, and opaque dust in the high-latitude area of LDN 1642. MATTILA K., VAISANEN P., LEHTINEN K., et al.

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