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Title:
High-Velocity Cloud Complex H: A Satellite of the Milky Way in a Retrograde Orbit?
Authors:
Lockman, Felix J.
Affiliation:
AA(National Radio Astronomy Observatory, P.O. Box 2, Green Bank, WV 24944-0002 )
Publication:
The Astrophysical Journal, Volume 591, Issue 1, pp. L33-L36. (ApJL Homepage)
Publication Date:
07/2003
Origin:
UCP
ApJ Keywords:
Galaxy: Halo, Galaxy: Structure, ISM: Clouds, Radio Lines: ISM
DOI:
10.1086/376961
Bibliographic Code:
2003ApJ...591L..33L

Abstract

Observations with the Green Bank Telescope of 21 cm H I emission from the high-velocity cloud complex H suggest that it is interacting with the Milky Way. A model in which the cloud is a satellite of the Galaxy in an inclined, retrograde circular orbit reproduces both the cloud's average velocity and its velocity gradient with latitude. The model places complex H at R=33+/-9 kpc from the Galactic center on a retrograde orbit inclined ~45° to the Galactic plane. At this location, it has a mass in H I of greater than 6×106 Msolar and dimensions of at least 10×5 kpc. Some of the diffuse H I associated with the cloud has apparently been decelerated by interaction with Galactic gas. Complex H has similarities to the dwarf irregular galaxy Leo A and to some compact high-velocity clouds, and it has an internal structure nearly identical to parts of the Magellanic Stream, with a pressure P/k~100 cm-3 K.
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