Titlebook: Nearby Molecular Clouds; Proceedings of a Spe Guy Serra Conference proceedings 1985 Springer-Verlag Berlin Heidelberg 1985 LOPES.astronomy.

Reservation

Galactic molecular clouds: Their size and mass distribution,e expressions are suggested to hold in the spiral arms of the Galaxy within galacto-centric distances 4.5 Kpc < R < 10 Kpc. In the interarm regions they must be truncated at r < 15 pc and M < 4 × 10. M. .

Compatriot

殘忍

流行

Large and small scale structures of molecular clouds in the taurus perseus complex, condensations of a few 100 MThe densest part of one of these condensations has a structure similar to that found in other dark clouds ?1 it is fragmented into several cores of a few Mo, with an orbital velocity dispersion ≈ 2 kms . In turn, the extended low-density layer, optically thick in CO (2-1

健談的人

消音器

Warm dust in the RCRA molecular cloud,nction. The 60–100 μm color temperature of this dust is 21 K. The 12–25 Jim color temperature is however 400 K. The emission of this warm dust extends over an area of 0.3 square degrees. This high temperature can not be explained by normal equilibrium processes. The only available heating source, th

Ingrained

Lecture Notes in Physicshttp://image.papertrans.cn/n/image/662320.jpg

GENRE

https://doi.org/10.1007/3-540-15991-6LOPES; astronomy; star; star formation

楓樹

978-3-540-15991-9Springer-Verlag Berlin Heidelberg 1985

TRAWL

Nearby Molecular Clouds978-3-540-39696-3Series ISSN 0075-8450 Series E-ISSN 1616-6361