Infall, Fragmentation and Outflow in Sgr B2

Details Infall, Fragmentation and Outflow in Sgr B2 Infall, Fragmentation and Outflow in Sgr B2

2006-08-10

arxiv.org/abs/astro-ph/0608213v1

Astronomy and Astrophysics

Astrophysics

5 pages, 3 figures, Published in J. Physics Conference Series

Scientific paper

10.1088/1742-6596/54/1/073

Observations of H$_{2}$CO lines and continuum at 1.3 mm towards Sgr B2(N) and Sgr B2(M) cores were carried out with the SMA. We imaged H$_{2}$CO line absorption against the continuum cores and the surrounding line emission clumps. The results show that the majority of the dense gas is falling into the major cores where massive stars have been formed. The filaments and clumps of the continuum and gas are detected outside of Sgr B2(N) and Sgr B2(M) cores. Both the spectra and moment analysis show the presence of outflows from Sgr B2(M) cores. The H$_{2}$CO gas in the red-shifted outflow of Sgr B2(M) appears to be excited by a non-LTE process which might be related to the shocks in the outflow.

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