Zobrazeno 1 - 4
of 4
pro vyhledávání: '"H. M. Butner"'
Autor:
H. J. Walker, H. M. Butner
Publikováno v:
Astrophysics and Space Science. 224:389-393
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::57f7e76d3832d8a076babcc7b095af72
https://doi.org/10.1007/bf00667877
https://doi.org/10.1007/bf00667877
Autor:
H. M. Butner
Publikováno v:
The Role of Dust in the Formation of Stars ISBN: 9783662225158
Thermal emission from dust provides us with a detailed loo at the overall temperature and density structure of a star-forming region, from the cold outer envelope to the hot inner disk. Much of our knowledge of the disk and envelope properties for yo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eba64bd6f248de9d228fbc237e5a6fea
https://doi.org/10.1007/978-3-540-68594-4_34
https://doi.org/10.1007/978-3-540-68594-4_34
Publikováno v:
Circumstellar Matter 1994 ISBN: 9789401040662
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d3dbc9a605d454f6ff60e0e2974f8f74
https://doi.org/10.1007/978-94-011-0147-9_14
https://doi.org/10.1007/978-94-011-0147-9_14
Publikováno v:
Light on Dark Matter ISBN: 9789401085779
The position of the emission peaks at 100 µm were compared with molecular clouds, identified using CO and HII regions.Data used were 1. IRAS spline data. The 60 °n and 100°m spline data were used (see Burton et al., 1986, for a description of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9a00eca7d0a028ddd85e4db29cfcd793
https://doi.org/10.1007/978-94-009-4672-9_79
https://doi.org/10.1007/978-94-009-4672-9_79