J/A+A/582/L12       V960 Mon light curves                    (Hackstein+, 2015)

Light curves of the lates FUor: Indications of a close binary. Hackstein M., Haas M., Kospal A., Hambsch F.-J., Chini R., Abraham P., Moor A., Pozo Nunez F., Ramolla M., Westhues C., Kaderhandt L., Fein C., Barr Dominguez A., Hodapp K.-W. <Astron. Astrophys. 582, L12 (2015)> =2015A&A...582L..12H 2015A&A...582L..12H (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Photometry, UBVRI ; Photometry, infrared ; Photometry, SDSS Keywords: stars: variables: T Tauri, Herbig Ae/Be - binaries: close - stars: individual: 2MASS J06593158-0405277 Abstract: We monitored the recent FUor 2MASS J06593158-0405277 (V960 Mon) since November 2009 at various observatories and multiple wavelengths. After the outburst by nearly 2.9mag in r around September 2014 the brightness gently fades until April 2015 by nearly 1mag in U and 0.5mag in z. Thereafter the brightness at λ>5000Å was constant until June 2015 while the shortest wavelengths (U,B) indicate a new rise, similar to that seen for the FUor V2493 Cyg (HBC722). Our near-infrared (NIR) monitoring between December 2014 and April 2015 shows a smaller outburst amplitude (∼2mag) and a smaller (0.2-0.3mag) post-outburst brightness decline. Optical and NIR color-magnitude diagrams indicate that the brightness decline is caused by growing extinction. The post-outburst light curves are modulated by an oscillating color-neutral pattern with a period of about 17 days and an amplitude declining from ∼0.08mag in October 2014 to ∼0.04mag in May 2015. The properties of the oscillating pattern lead us to suggest the presence of a close binary with eccentric orbit. Description: Photometric light curves for V960Mon (2MASS J06593158-0405277) from different telescopes at multiple wavelengths between September 2009 to June 2015. This comprises optical observations from Universitaetssternwarte Bochum (USB) in Chile as part of the Bochum Galatic Disk Survey (GDS, 2015AN....336..590H 2015AN....336..590H), Konkoly Observatory in Hungary, and the Remote Observatory Atacama Desert (ROAD) in Chile, as well as near-infrared data from USB. Objects: ------------------------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------------------------ 06 59 31.58 -04 05 27. 7 V960Mon = 2MASS J06593158-0405277 ------------------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file lc_data.dat 40 1376 Light curves of V960 Mon -------------------------------------------------------------------------------- See also: J/A+AS/124/33 : BN Ori UBV photometry + equivalent width (Shevchenko+ 1997) J/A+A/556/A60 : BVRI observations of the FUor star V582 Aur (Semkov+, 2013) Byte-by-byte Description of file: lc_data.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Tel Telescope 13- 23 F11.5 d MJD Modified Julian Date 25 A1 --- Filt [UBVRIJHKriz] Filter (1) 27- 33 F7.4 mag mag Magnitude in filter 35- 40 F6.4 mag e_mag rms uncertainty on mag -------------------------------------------------------------------------------- Note (1): Filters informations as follows: UBVRI = Johnson-Cousins riz = Sloan JHK = 2MASS J,H,Ks -------------------------------------------------------------------------------- Acknowledgements: Moritz Hackstein, hackstein(at)astro.rub.de
(End) Moritz Hackstein [AIRUB], Patricia Vannier [CDS] 08-Oct-2015
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line