The polar Catalysmic Variable 1RXS J173006.4+033813

2); (2) Univ. of Toronto; (3) Space Radiation Lab - Caltech); Fiona A. Harrison (3); Mansi M. Kasliwal (1); Marten H. van Kerkwijk (1; S. R. Kulkarni (1); Varun B. Bhalerao (1); Vikram R. Rana (3) ((1) Caltech

REVIEW

The polar Catalysmic Variable 1RXS J173006.4+033813

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 1008.2002 v1 pith:ERR3FBET submitted 2010-08-11 astro-ph.SR

The polar Catalysmic Variable 1RXS J173006.4+033813

Varun B. Bhalerao (1) , Marten H. van Kerkwijk (1 , 2) , Fiona A. Harrison (3) , Mansi M. Kasliwal (1) , S. R. Kulkarni (1) , Vikram R. Rana (3) ((1) Caltech , (2) Univ. of Toronto

show 1 more author

(3) Space Radiation Lab - Caltech)

This is my paper

classification astro-ph.SR

keywords dwarfj173006modulationpolarsecondaryvariableactivearise

verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved

0 comments

read the original abstract

We report the discovery of 1RXS J173006.4+033813, a polar cataclysmic variable with a period of 120.21 min. The white dwarf primary has a magnetic field of B = 42+6-5 MG, and the secondary is a M3 dwarf. The system shows highly symmetric double peaked photometric modulation in the active state as well as in quiescence. These arise from a combination of cyclotron beaming and ellipsoidal modulation. The projected orbital velocity of the secondary is K2 = 390+-4 km/s. We place an upper limit of 830+-65 pc on the distance.

The polar Catalysmic Variable 1RXS J173006.4+033813

discussion (0)