Pith. sign in

REVIEW

OGLE-BLG182.1.162852: An Eclipsing Binary with a Circumstellar Disk

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 1410.2643 v1 pith:SF3ZL2YJ submitted 2014-10-09 astro-ph.SR

OGLE-BLG182.1.162852: An Eclipsing Binary with a Circumstellar Disk

N. J. Rattenbury , {\L}. Wyrzykowski , Z. Kostrzewa-Rutkowska , A. Udalski , S. Koz{\l}owski , M. K. Szyma\'nski , G. Pietrzy\'nski , I. Soszy\'nski
show 6 more authors
R. Poleski K. Ulaczyk J. Skowron P. Pietrukowicz P. Mr\'oz D. Skowron
This is my paper
classification astro-ph.SR
keywords dimmingogle-blg182curvediskeventlightsystembinary
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

We present the discovery of a plausible disk-eclipse system OGLE-BLG182.1.162852. The OGLE light curve for OGLE-BLG182.1.162852 shows three episodes of dimming by $I \simeq 2 - 3$ magnitudes, separated by 1277 days. The shape of the light curve during dimming events is very similar to that of known disk eclipse system OGLE-LMC-ECL-11893 (Dong et al. 2014). The event is presently undergoing a dimming event, predicted to end on December 30th, 2014. We encourage spectroscopic and multi-band photometric observations now. The next dimming episode for OGLE-BLG182.1.162852 is expected to occur in March 2018.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.