Titlebook: Dense Molecular Gas around Protostars and in Galactic Nuclei; European Workshop on W.A. Baan,Y. Hagiwara,H.J. Langevelde Book 2005 Springer

有害

https://doi.org/10.1057/9781137415547otions exhibit outflows, which likely originate from two of the hyper-compact HII regions in this source. Sarma et al., have detected the Zeeman effect in water masers toward W3 IRS5 and measured line-of-sight magnetic field strengths of between 14 and 42 mG. The directions of maser linear polarizat

esthetician

Domestic Dog Cognition and Behaviorars. There is also convincing evidence for relations between the properties of supermassive black holes in the nuclei of galaxies and those of their host galaxies. It is much less clear, however, how stellar starburstt) and non-stellar (AGN) activity in the nuclear regions can be initiated and fuell

constellation

冥界三河

remission

Clinton L. Beckford,Donovan R. Campbellngle-dish monitoring and high-resolution interferometry have been used to identify sites of massive star formation, to study the interaction of nuclear jets with dense molecular gas and to investigate the circumnuclear environment of active galactic nuclei (AGN). Accretion disks with radii of 0.1–3

Condense

Clinton L. Beckford,Donovan R. Campbelled as a part of a small sample of FR II galaxies with evidence of nuclear obscuration. The isotropic luminosity of the maser is ∼1200 .ʘ. With a recessional velocity of cz ∼- 17680 km s. it is the most distant water maser so far reported. The line arises from the densest (>10. cm .) interstellar gas

Charade

改变立场