CaltechAUTHORS
  A Caltech Library Service

Hunting for millimeter flares from magnetic reconnection in pre-main sequence spectroscopic binaries

Kóspál, Á. and Salter, D. M. and Hogerheijde, M. R. and Moór, A. and Blake, G. A. (2011) Hunting for millimeter flares from magnetic reconnection in pre-main sequence spectroscopic binaries. Astronomy and Astrophysics, 527 . Art. No. A96. ISSN 0004-6361. https://resolver.caltech.edu/CaltechAUTHORS:20110323-082110941

[img]
Preview
PDF - Published Version
See Usage Policy.

994Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20110323-082110941

Abstract

Context. Recent observations of the low-mass pre-main sequence (PMS), eccentric spectroscopic binaries DQ Tau and V773 Tau A reveal that their millimeter spectrum is occasionally dominated by flares from non-thermal emission processes. The transient activity is believed to be synchrotron in nature, resulting from powerful magnetic reconnection events when the separate magnetic structures of the binary components are briefly capable of interacting and forced to reorganize, typically near periastron. Aims. We conducted the first systematic study of the millimeter variability toward a sample of 12 PMS spectroscopic binaries with the aim to characterize the proliferation of flares amongst sources likely to experience similar interbinary reconnection events. The source sample consists entirely of short-period, close-separation binaries that possess either a high orbital eccentricity (e > 0.1) or a circular orbit (e ≈ 0). Methods. Using the MAMBO2 array on the IRAM 30 m telescope, we carried out continuous monitoring at 1.25mm (240GHz) over a 4-night period during which all of the high-eccentricity binaries approached periastron. We also obtained simultaneous optical VRI measurements, since a strong link is often observed between stellar reconnection events (traced via X-rays) and optical brightenings. Results. UZ Tau E is the only source to be detected at millimeter wavelengths, and it exhibited significant variation (F_(1.25mm) = 87– 179 mJy); it is also the only source to undergo strong simultaneous optical variability (ΔR ≈ 0.9 mag). The binary possesses the largest orbital eccentricity in the current sample, a predicted factor in star-star magnetic interaction events. With orbital parameters and variable accretion activity similar to DQ Tau, the millimeter behavior of UZ Tau E draws many parallels to the DQ Tau model for colliding magnetospheres. However, on the basis of our observations alone, we cannot determine whether the variability is repetitive, or if it could also be due to variable free-free emission in an ionized wind. Conclusions. UZ Tau E brings the number of known millimeter-varying PMS sources to 3 out of a total of 14 monitored binaries now in the literature. Important factors in the non-detection of the rest of our targets are the coarse time-sampling and limited millimeter sensitivity of our survey. We recommend that future studies concentrate on close-by targets, and obtain millimeter and optical data points with better temporal resolution.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/0004-6361/201015917DOIArticle
http://www.aanda.org/index.php?option=com_article&access=doi&doi=10.1051/0004-6361/201015917&Itemid=129PublisherArticle
ORCID:
AuthorORCID
Blake, G. A.0000-0003-0787-1610
Additional Information:© 2011 ESO. Received 12 October 2010, Accepted 17 December 2010, Published online 01 February 2011. Based on observations with the IRAM 30 m telescope at Pico Veleta (Spain). IRAM is funded by the INSU/CNRS (France), the MPG (Germany) and the IGN (Spain). Appendix is only available in electronic form at http://www.aanda.org. This article publishes observations made with the IAC- 80 telescope, operated by the Instituto de Astrofísica de Canarias at the Teide Observatory (Spain), and with the Schmidt telescope at the Piszkéstető Mountain Station of the Konkoly Observatory (Hungary); we are grateful for the granted telescope time. We thank C. Zurita Espinosa for obtaining the IAC-80 data as part of a routine observing program. We are also grateful to B. Ocaña and J. Santiago for their help during the IRAM 30m observations. The research of Á.K., D.M.S., and M.R.H. is supported by the Nederlands Organization for Scientific Research (NWO). This work has benefited from research funding from the European Community’s Seventh Framework Programme under RadioNet.
Funders:
Funding AgencyGrant Number
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)UNSPECIFIED
European CommunityUNSPECIFIED
Subject Keywords:stars: pre-main sequence – binaries: spectroscopic – stars: variables: general – radio continuum: stars – stars: flare – stars: individual: UZ Tau E
Record Number:CaltechAUTHORS:20110323-082110941
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20110323-082110941
Official Citation:Hunting for millimeter flares from magnetic reconnection in pre-main sequence spectroscopic binaries Á. Kóspál, D. M. Salter, M. R. Hogerheijde, A. Moór and G. A. Blake A&A 527 A96 (2011) DOI: 10.1051/0004-6361/201015917
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:23067
Collection:CaltechAUTHORS
Deposited By: Benjamin Perez
Deposited On:23 Mar 2011 15:59
Last Modified:03 Oct 2019 02:43

Repository Staff Only: item control page