CaltechAUTHORS
  A Caltech Library Service

A Survey of the High Order Multiplicity of Nearby Solar-type Binary Stars with Robo-AO

Riddle, Reed L. and Tokovinin, Andrei and Mason, Brian D. and Hartkopf, William I. and Roberts, Lewis C., Jr. and Baranec, Christoph and Law, Nicholas M. and Bui, Khanh and Burse, Mahesh P. and Das, H. K. and Dekany, Richard G. and Kulkarni, Shrinivas and Punnadi, Sujit and Ramaprakash, A. N. and Tendulkar, Shriharsh P. (2015) A Survey of the High Order Multiplicity of Nearby Solar-type Binary Stars with Robo-AO. Astrophysical Journal, 799 (1). Art. No. 4. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20150226-150321481

[img] PDF - Published Version
See Usage Policy.

1537Kb
[img] PDF - Submitted Version
See Usage Policy.

1638Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20150226-150321481

Abstract

We conducted a survey of nearby binary systems composed of main sequence stars of spectral types F and G in order to improve our understanding of the hierarchical nature of multiple star systems. Using Robo-AO, the first robotic adaptive optics instrument, we collected high angular resolution images with deep and well-defined detection limits in the Sloan Digital Sky Survey i' band. A total of 695 components belonging to 595 systems were observed. We prioritized observations of faint secondary components with separations over 10" to quantify the still poorly constrained frequency of their subsystems. Of the 214 secondaries observed, 39 contain such subsystems; 19 of those were discovered with Robo-AO. The selection-corrected frequency of secondary subsystems with periods from 10^(3.5) to 10^5 days is 0.12 ± 0.03, the same as the frequency of such companions to the primary. Half of the secondary pairs belong to quadruple systems where the primary is also a close pair, showing that the presence of subsystems in both components of the outer binary is correlated. The relatively large abundance of 2+2 quadruple systems is a new finding, and will require more exploration of the formation mechanism of multiple star systems. We also targeted close binaries with periods less than 100 yr, searching for their distant tertiary components, and discovered 17 certain and 2 potential new triples. In a subsample of 241 close binaries, 71 have additional outer companions. The overall frequency of tertiary components is not enhanced, compared to all (non-binary) targets, but in the range of outer periods from 106 to 107.5 days (separations on the order of 500 AU), the frequency of tertiary components is 0.16 ± 0.03, exceeding the frequency of similar systems among all targets (0.09) by almost a factor of two. Measurements of binary stars with Robo-AO allowed us to compute first orbits for 9 pairs and to improve orbits of another 11 pairs.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/799/1/4DOIArticle
http://iopscience.iop.org/0004-637X/799/1/4/PublisherArticle
http://arxiv.org/abs/1411.0682arXivDiscussion Paper
ORCID:
AuthorORCID
Riddle, Reed L.0000-0002-0387-370X
Roberts, Lewis C., Jr.0000-0003-3892-2900
Baranec, Christoph0000-0002-1917-9157
Law, Nicholas M.0000-0001-9380-6457
Kulkarni, Shrinivas0000-0001-5390-8563
Tendulkar, Shriharsh P.0000-0003-2548-2926
Additional Information:© 2015 American Astronomical Society. Received 2014 July 30; accepted 2014 November 1; published 2015 January 9. We acknowledge the input of the referee who read through this lengthy paper and gave us comments to improve it. The Robo-AO system is supported by collaborating partner institutions, the California Institute of Technology and the Inter-University Centre for Astronomy and Astrophysics, and by the National Science Foundation under grant Nos. AST-0906060, AST-0960343, and AST-1207891, by the Mount Cuba Astronomical Foundation, and by a gift from Samuel Oschin. We are grateful to the Palomar Observatory staff for their ongoing support of Robo-AO on the P60, particularly S. Kunsman, M. Doyle, J. Henning, R. Walters, G. Van Idsinga, B. Baker, K. Dunscombe and D. Roderick. A portion of the research in this paper was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. C.B. acknowledges support from the Alfred P. Sloan Foundation. This work used the SIMBAD service operated by Centre des Données Stellaires (Strasbourg, France), bibliographic references from the Astrophysics Data System maintained by SAO/NASA, data products of the Two Micron All-Sky Survey (2MASS), the Washington Double Star Catalog maintained at USNO. Facility: PO:1.5m (Robo-AO)
Funders:
Funding AgencyGrant Number
CaltechUNSPECIFIED
Inter-University Centre for Astronomy and AstrophysicsUNSPECIFIED
NSFAST-0906060
NSFAST-0960343
NSFAST-1207891
Mount Cuba Astronomical FoundationUNSPECIFIED
Samuel OschinUNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Alfred P. Sloan FoundationUNSPECIFIED
Subject Keywords:binaries: close; binaries: general; instrumentation: adaptive optics; stars: formation; techniques: high angular resolution
Issue or Number:1
Record Number:CaltechAUTHORS:20150226-150321481
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150226-150321481
Official Citation:A Survey of the High Order Multiplicity of Nearby Solar-type Binary Stars with Robo-AO Reed L. Riddle et al. 2015 ApJ 799 4
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:55276
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:26 Feb 2015 23:27
Last Modified:09 Mar 2020 13:19

Repository Staff Only: item control page