Observations of Complex H, a High Velocity Cloud Close to the Galactic Plane

Bibcode
2008ASPC..390..384B
Buenrostro, V.; Lockman, J.; Beckman, J. E.
Bibliographical reference

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at Santiago del Teide, Tenerife, Spain. Edited by J. H. Knapen, T. J. Mahoney, and A. Vazdekis San Francisco: Astronomical Society of the Pacific, 2008., p.384

Advertised on:
6
2008
Number of authors
3
IAC number of authors
0
Citations
1
Refereed citations
1
Description
Using 21 cm observations of Complex H with the Green Bank Radio Telescope, we have derived its LSR velocity of ˜ 200 km s-1 and an H I mass of 7.5× 107 M&sun;. This gives useful support to the scenario in which the Galactic disk is being built up by the continual accretion of clouds of this type from the intracluster medium of the Local Group. Complex H is detected as shedding a gas tail, and has a shock front at its leading surface, both phenomena attributable to its interaction with the halo gas of the Milky Way.
Type
Non-refereed

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