Figure 10 from Near-Infrared Imaging Polarimetry of M42: Aperture Polarimetry of Point-Like Sources

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Near-Infrared Imaging Polarimetry of M42: Aperture Polarimetry of Point-Like Sources

Authors: Nobuhiko Kusakabe, Motohide Tamura, Ryo Kandori, Jun Hashimoto, Yasushi Nakajima, Tetsuya Nagata, Takahiro Nagayama, Jim Hough, and Phil Lucas

KUSAKABE et al. 2008 The Astronomical Journal 136 621.

Provider: AAS Journals

Caption: Figure 10.

P( H)/ A( H) for the 28 sources cross-identified with Slesnick et al. (2004) (filled circle) and Riddick et al. (2007) (open circle). The horizontal line indicates P( H)/ A( H) = 2.9, which corresponds to the assumed maximum value for interstellar polarization. The broken line indicates 0.08 M _☉, which corresponds to the brown dwarf mass limit.

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