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Ysovar: The First Sensitive, Wide-area, Mid-infrared Photometric Monitoring of the Orion Nebula Cluster

Morales-Calderón, M. and Stauffer, J. R. and Hillenbrand, L. A. and Rebull, L. M. and Carpenter, J. M. and Plavchan, P. and Ardila, D. R. (2011) Ysovar: The First Sensitive, Wide-area, Mid-infrared Photometric Monitoring of the Orion Nebula Cluster. Astrophysical Journal, 733 (1). Art. No. 50. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20110531-153620935

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Abstract

We present initial results from time-series imaging at infrared wavelengths of 0.9 deg^2 in the Orion Nebula Cluster (ONC). During Fall 2009 we obtained 81 epochs of Spitzer 3.6 and 4.5 μm data over 40 consecutive days. We extracted light curves with ~3% photometric accuracy for ~2000 ONC members ranging from several solar masses down to well below the hydrogen-burning mass limit. For many of the stars, we also have time-series photometry obtained at optical (I_c) and/or near-infrared (JK_s ) wavelengths. Our data set can be mined to determine stellar rotation periods, identify new pre-main-sequence eclipsing binaries, search for new substellar Orion members, and help better determine the frequency of circumstellar disks as a function of stellar mass in the ONC. Our primary focus is the unique ability of 3.6 and 4.5 μm variability information to improve our understanding of inner disk processes and structure in the Class I and II young stellar objects (YSOs). In this paper, we provide a brief overview of the YSOVAR Orion data obtained in Fall 2009 and highlight our light curves for AA-Tau analogs—YSOs with narrow dips in flux, most probably due to disk density structures passing through our line of sight. Detailed follow-up observations are needed in order to better quantify the nature of the obscuring bodies and what this implies for the structure of the inner disks of YSOs.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/733/1/50DOIArticle
http://iopscience.iop.org/0004-637X/733/1/50PublisherArticle
ORCID:
AuthorORCID
Stauffer, J. R.0000-0003-3595-7382
Rebull, L. M.0000-0001-6381-515X
Carpenter, J. M.0000-0003-2251-0602
Plavchan, P.0000-0002-8864-1667
Additional Information:© 2011 American Astronomical Society. Received 2011 March 16; accepted 2011 March 16; published 2011 May 3. We thank the anonymous referee for her helpful comments. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This work is also based (in part) on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, and the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Facility: Spitzer (IRAC)
Group:Infrared Processing and Analysis Center (IPAC)
Subject Keywords:circumstellar matter; open clusters and associations: individual (Orion); stars: pre-main sequence; stars: protostars; stars: variables: general
Issue or Number:1
Classification Code:PACS: 98.20.Di; 95.85.Hp; 98.38.Dq; 97.10.Fy; 97.10.Ri; 97.21.+a
Record Number:CaltechAUTHORS:20110531-153620935
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20110531-153620935
Official Citation:Ysovar: The First Sensitive, Wide-area, Mid-infrared Photometric Monitoring of the Orion Nebula Cluster M. Morales-Calderón et al. 2011 ApJ 733 50
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:23846
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:01 Jun 2011 14:50
Last Modified:09 Mar 2020 13:18

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