Dynamics of Ionized Gas at the Galactic Center: VLA Observations of the 3D Velocity Field and Location of the Ionized Streams in Sagittarius A West

Details Dynamics of Ionized Gas at the Galactic Center: VLA Observations of the 3D Velocity Field and Location of the Ionized Streams in Sagittarius A West Dynamics of Ionized Gas at the Galactic Center: VLA Observations of the 3D Velocity Field and Location of the Ionized Streams in Sagittarius A West

2009-04-20

arxiv.org/abs/0904.3133v2

Astrophys.J.699:186-214,2009

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

62 pages, 22 figures, ApJ in press

Scientific paper

10.1088/0004-637X/699/1/186

We present new results based on high-resolution observations of Sgr A West at the Galactic center with the VLA at 1.3 cm. We measured proper motions for 71 compact HII components. We also investigated radial velocities in the LSR velocity using the H92a line data. Combining proper motion and radial velocity measurements, we have determined the 3D velocity distribution in Sgr A West. We find that the three ionized streams (Northern Arm, Eastern Arm, and Western Arc) can be modeled with three bundles of Keplerian orbits around Sgr A*. We determined the five orbital parameters for each of them using LSQ fitting to the locii of the streams. Our results confirm earlier results on the streams in the Western Arc and the Northern Arm to be in Keplerian orbits, suggesting that the stream in the Eastern Arm is also consistent with an elliptical orbit. Both the Northern and Eastern Arm streams have high eccentricities, while the Western Arc stream is nearly circular. All three streams orbit around Sgr A* in a counterclockwise sense (viewed from the Earth). We also report an ionized nebula associated with IRS 8, including a bow shock in radio continuum emission which shows excellent agreement with near IR observations. From the H92a line data, we find evidence for interaction between the IRS 8 nebula and the Northern Arm stream. Other new morphological features revealed in our high-resolution image include: 1) a helical structure in the Northern Arm, suggesting that MHD plays an important role in the motion of the ionized gas, in addition to the dynamics determined by the central gravitational field and 2) a linear feature in the IRS 16 region, suggesting the compressed edge of the Northern Arm may result from the collective winds and radiation pressure from the high mass stars in the IRS16 cluster.

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