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

蛤肉

信徒

不舒服

High-Resolution Observations in B1-IRS: Ammonia, CCS and Water Masers high angular resolution (∼4″). We have used VLA observations of NH., CCS, and H.O masers at 1 cm. CCS emission shows three clumps around the central source, with a velocity gradient from red to blue-shifted velocities towards the protostar, probably due to the interaction with outflowing material.

Aromatic

好开玩笑

Gravitationally Induced Inflow in Starbursts and AGNars. 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

ellagic-acid

Feeding Monsters — A Study of Active Galaxiesr resolution and high sensitivity carried out with the IRAM Plateau de Bure interferometer (PdBI). The observations cover galaxies in a redshift range of ∼0.03–1.4. We have so far observed five different active galaxies: NGC3718, NGC1068, HE1029-1831, 3C48 and Q0957 + 561. The first two objects belo

EVEN

The QSO Hosts I Zw 1 and 3C 48: Prototypes of a Merger-Driven Quasar Evolution?rared galaxies (ULIRGs) to quasi-stellar objects (QSOs). Since galaxy mergers are assumed to trigger the evolution, it is important to confirm the merger properties of transitionary objects. Using multi-wavelength observations and N-body simulations, the merger histories of I Zw 1 and 3C 48 have bee

cancellous-bone

是突袭

Corporeal

Dense Gas, Chemistry and Star Formation in Luminous Galaxiestution of the molecular gas will change with, and respond to, the evolution of the activity. This paper includes a short discussion of the .CO/.CO 1-0 line intensity ratio as a diagnostic tool of the molecular gas properties of luminous galaxies — paired with examples of high-resolution studies of h