Pith. sign in

REVIEW

Clumpy molecular structures revolving the B[e] supergiant MWC 137

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 1610.05596 v1 pith:K367K4OK submitted 2016-10-17 astro-ph.SR

M. Kraus , L.S. Cidale , T. Liimets , C.E. Cappa , N. Duronea , D.S. Gunawan , M.E. Oksala , M. Santander-Garcia
show 5 more authors
M.L. Arias D.H. Nickeler G. Maravelias M. Borges Fernandes M. Cure
This is my paper
classification astro-ph.SR
keywords clumpymolecularnebulaopticalstarstructuressupergiantapex
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

The peculiar emission-line star MWC 137 with its extended optical nebula was recently classified as B[e] supergiant. To study the spatial distribution of its circumstellar molecular gas on small and large scales, we obtained near-infrared and radio observations using SINFONI and APEX, respectively. We find that the hot CO gas is arranged in moving clumpy ring and shell structures close to the star, while a cold CO envelope is encircling the borders of the optical nebula from the south to the west.

Discussion (0). Sign in to comment.

Pith tools