The ALMA View of the OMC1 Explosion in Orion

The ALMA View of the OMC1 Explosion in Orion

Most massive stars form in dense clusters where gravitational interactions with other. stars may be common. The two nearest forming massive stars, the BN object and Source I, located behind the Orion Nebula, were ejected with velocities of similar to 29 and similar to 13 km s(-1) about 500 years ago...

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Bibliographic Details
Main Authors: Bally, John, Ginsburg, Adam, Arce, Hector, Eisner, Josh, Youngblood, Allison, Zapata, Luis, Zinnecker, Hans
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
Herbig-Haro objects - ISM
individual objects (Orion OMC1) - ISM
jets and outflows stars - stars
formation -stars
massive
Online Access:http://hdl.handle.net/10150/623202
http://arizona.openrepository.com/arizona/handle/10150/623202

Internet

http://hdl.handle.net/10150/623202
http://arizona.openrepository.com/arizona/handle/10150/623202

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