Figure 3 from A Chandra Study of the Rosette Star-Forming Complex. II. Clusters in the Rosette Molecular Cloud

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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 3.

Variable X-ray light curve of ACIS source #119. The KS test finds a significant variation ( P _KS ⩽ 0.005), but no flaring characterized by fast rise and slow decay as commonly seen in PMS stars is present.

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