4.7 Article

THE GOULD'S BELT DISTANCES SURVEY (GOBELINS). II. DISTANCES AND STRUCTURE TOWARD THE ORION MOLECULAR CLOUDS

期刊

ASTROPHYSICAL JOURNAL
卷 834, 期 2, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4357/834/2/142

关键词

astrometry; ISM: individual objects (Orion Molecular Clouds); parallaxes; radiation mechanisms: nonthermal; stars: kinematics and dynamics

资金

  1. DGAPA
  2. UNAM
  3. CONACyT, Mexico
  4. von Humboldt Stiftung
  5. NSF [AST-1109116]
  6. FAPESP

向作者/读者索取更多资源

We present the results of the Gould's Belt Distances Survey of young star-forming regions toward the Orion Molecular Cloud Complex. We detected 36 young stellar objects (YSOs) with the Very Large Baseline Array, 27 of which have been observed in at least three epochs over the course of two years. At least half of these YSOs belong to multiple systems. We obtained parallax and proper motions toward these stars to study the structure and kinematics of the Complex. We measured a distance of 388 +/- 5 pc toward the Orion Nebula Cluster, 428 +/- 10 pc toward the southern portion L1641, 388 +/- 10 pc toward NGC 2068, and roughly similar to 420 pc toward NGC 2024. Finally, we observed a strong degree of plasma radio scattering toward lambda Ori.

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