... SWAS: found · Water vapor is present in almost all star-forming regions · Gas-phase water abundance peaks near molecular surfaces; · Molecularclouds have an abundance of water-ice in their interiors . ...
... in the strength of background O emission have been noted (tentatively) in repeated Chandra observations of MBM 12, a nearby dark molecularcloud that shadows much of the SXRB (R. J. Edgar et al. 2004, in preparation), and in XMM-Newton observations of the ...
... In the coldest regions the material consists of molecular gas and dust; in the hottest regions the material is almost ... The Diffuse ISM High-Latitude Clouds A. Goodman . Mapping out Dust in the Dense ISM A. Goodman . ...
... 1999), H ii regions from Hodge et al. (1999), giant molecularclouds from Engargiola et al. (2003), globular clusters from Mochejska et al. (1998), star clusters No. ...
... been used often in astronomical wavelet analyses,7 in, for example : the analysis of 13CO spectral maps of the molecularcloud L1551 (Gill & Henrikson 1990 ; see also Langer, Wilson, & Anderson 1993, who apply Laplacian pyramid transforms to a 13CO image ...
[
Текст
]
Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1112/2002ApJS..138..185F.pdf -- 940.2 Кб -- 07.02.2012 Похожие документы