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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 7.

Surface density contours based on 10th neighbor distances for the Chandra RMC sources. The green contours are densities for all candidates. The blue lines are contours for unobscured sources ( medE ⩽ 2.0 keV), and the red lines are contours for obscured sources ( medE > 2.0 keV). All contours follow the levels of density for obscured sources, starting at 0.057 stars arcmin −2 with steps of 0.45 stars arcmin −2.

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