M. Morales-Calderon, J. R. Stauffer, L. A. Hillenbrand, R. Gutermuth, I. Song, L. M. Rebull, P. Plavchan, J. M. Carpenter, B. A. Whitney, K. Covey, C. Alves de Oliveira, E. Winston, M. J. McCaughrean, J. Bouvier, S. Guieu, F. J. Vrba, J. Holtzman, F. Marchis, J. L. Hora, L. H. WassermanS. Terebey, T. Megeath, E. Guinan, J. Forbrich, N. Huelamo, P. Riviere-Marichalar, D. Barrado, K. Stapelfeldt, J. Hernandez, L. E. Allen, D. R. Ardila, A. Bayo, F. Favata, D. James, M. Werner, K. Wood

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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 mu m data over 40 consecutive days. We extracted light curves with similar to 3% photometric accuracy for similar to 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 mu m 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.

Original languageEnglish
Article number50
Number of pages9
JournalAstrophysical Journal
Issue number1
Publication statusPublished - 20 May 2011


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