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A Chandra Study of the Rosette Star-Forming Complex. II. Clusters in the Rosette Molecular Cloud

  • Authors: Junfeng Wang, Eric D. Feigelson, Leisa K. Townsley, Carlos G. Román-Zúñiga, Elizabeth Lada, and Gordon Garmire

WANG et al. 2009 The Astrophysical Journal 696 47.

  • Provider: AAS Journals

Caption: Figure 11.

NIR JH vs. HK color–color diagram for Chandra stars with high-quality JHK photometry (error in both JH and HK colors <0.1 mag) in regions A, B, and C as defined in Figure  7. The green circles and red triangles represent sources with and without significant K-band excess ( E( HK)>2σ( HK)), respectively. The black solid and long-dashed lines denote the loci of MS stars and giants, respectively, from Bessell & Brett (1988). The purple dash-dotted line is the locus for classical T Tauri stars from Meyer et al. (1997), and the cyan solid line is the locus for HAeBe stars from Lada & Adams (1992). The blue dashed lines represent the standard reddening vector with crosses marking every A V = 5 mag.

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