Pith. sign in

REVIEW

The Gould's Belt Distances Survey (GOBELINS) II. Distances and structure towards the Orion Molecular Clouds

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1609.04041 v2 pith:CUGCSFKV submitted 2016-09-13 astro-ph.SR astro-ph.GA

Marina Kounkel , Lee Hartmann , Laurent Loinard , Gisela N. Ortiz-León , Amy J. Mioduszewski , Luis F. Rodríguez , Sergio A. Dzib , Rosa M. Torres
show 7 more authors
Gerardo Pech Phillip A. B. Galli Juana L. Rivera Andrew F. Boden Neal J. Evans II Cesar Briceño John J. Tobin
This is my paper
classification astro-ph.SRastro-ph.GA
keywords towardsdistancesorionbeltcomplexgobelinsgouldleast
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

We present the results of the Gould's Belt Distances Survey (GOBELINS) of young star forming regions towards the Orion Molecular Cloud Complex. We detected 36 YSOs with the Very Large Baseline Array (VLBA), 27 of which have been observed in at least 3 epochs over the course of 2 years. At least half of these YSOs belong to multiple systems. We obtained parallax and proper motions towards these stars to study the structure and kinematics of the Complex. We measured a distance of 388$\pm$5 pc towards the Orion Nebula Cluster, 428$\pm$10 pc towards the southern portion L1641, 388$\pm$10 pc towards NGC 2068, and roughly $\sim$420 pc towards NGC 2024. Finally, we observed a strong degree of plasma radio scattering towards $\lambda$ Ori.

Discussion (0). Sign in to comment.

Pith tools