An HST survey for 100–1000 au companions around young stellar objects in the Orion molecular clouds: Evidence for environmentally dependent multiplicity
- Department of Astronomy, University of Michigan, Ann Arbor, MI 48109 (United States)
- Ritter Astrophysical Research Center, Department of Physics and Astronomy, University of Toledo, Toledo, OH 43606 (United States)
- New York Center for Astrobiology, Rensselaer Polytechnic Institute, Troy, NY (United States)
- NASA Postdoctoral Program Fellow, Goddard Space Flight Center, Greenbelt, MD (United States)
We present a near-infrared survey for the visual multiples in the Orion molecular clouds region at separations between 100 and 1000 au. These data were acquired at 1.6 μm with the NICMOS and WFC3 cameras on the Hubble Space Telescope. Additional photometry was obtained for some of the sources at 2.05 μm with NICMOS and in the L′ band with NSFCAM2 on NASA’s InfraRed Telescope Facility. Toward 129 protostars and 197 pre-main-sequence stars with disks observed with WFC3, we detect 21 and 28 candidate companions between the projected separations of 100–1000 au, of which less than 5 and 8, respectively, are chance line-of-sight coincidences. The resulting companion fraction (CF) after the correction for the line-of-sight contamination is 14.4{sub −1.3}{sup +1.1}% for protostars and 12.5{sub −0.8}{sup +1.2}% for the pre-main-sequence stars. These values are similar to those found for main-sequence stars, suggesting that there is little variation in the CF with evolution, although several observational biases may mask a decrease in the CF from protostars to the main-sequence stars. After segregating the sample into two populations based on the surrounding surface density of young stellar objects, we find that the CF in the high stellar density regions (Σ{sub YSO} > 45 pc{sup −2}) is approximately 50% higher than that found in the low stellar density regions (Σ{sub YSO} < 45 pc{sup −2}). We interpret this as evidence for the elevated formation of companions at 100–1000 au in the denser environments of Orion. We discuss possible reasons for this elevated formation.
- OSTI ID:
- 22890073
- Journal Information:
- Astrophysical Journal, Vol. 821, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); Since 2009, the country of publication for this journal is the UK.; ISSN 0004-637X
- Country of Publication:
- United Kingdom
- Language:
- English
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