Miju Kang et al. 2008 ApJ 683 267 doi:10.1086/589819
Millimeter Imaging of HH 24 MMS: A Misaligned Protobinary System
FREE ISSUEMiju Kang1,2,3, Minho Choi1, Paul T. P. Ho4,5 and Youngung Lee1
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. Disk masses of sources 1 and 2 are 0.6 and 0.3 M, respectively. Both sources are highly elongated. The difference in the position angle of the two disks is ~45°, which means that HH 24 MMS is a highly misaligned protobinary system. The misalignment suggests that turbulent fragmentation may be the formation mechanism relevant to the binary systems with a separation of a few hundreds of AU, such as the HH 24 MMS system.
- Subject headings
accretion, accretion disks; binaries: general; ISM: individual (HH 24 MMS); ISM: structure; stars: formation
- Dates
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Issue 1 (2008 August 10)
Received 2007 August 14, accepted for publication 2008 April 30
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Millimeter Imaging of HH 24 MMS: A Misaligned Protobinary System
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