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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 10.

Spatial distribution of all the IR counterparts to our X-ray sources. The dense molecular cloud is outlined by the 12CO emission contours (Heyer et al. 2006). Overlaid red polygons are the regions A, B, and C defined by X-ray source densities, and the symbols are the X-ray-selected stars classified as Class I (magenta circles), Class II (green diamonds), and Class III (black crosses) based on their NIR colors. The O7 star and the Class I protostar RMCX #89 are labeled. The overall distribution of the Class II/I sources is more confined to the CO molecular ridge than the Class III stars.

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