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X‐Ray and Radio Observations of the Cygnus OB2 Association

  • Authors: Wayne L. Waldron , Michael F. Corcoran, Stephen A. Drake, and Alan P. Smale

Waldron et al. 1998 The Astrophysical Journal Supplement Series 118 217.

  • Provider: AAS Journals

Caption: Fig. 3.

Confidence contours (68%, 90%, and 99%) in the log TX vs. log NH(ISM) plane for the ISM model (cold absorber). The open and filled circles mark the best‐fit parameters (see Table 4). The dashed lines and open symbols represent the confidence contours and best fits for the low S/N observation (1991 April 21), whereas the solid lines and filled symbols represent the confidence contours and best fits for the high S/N observation (1993 April 29). The solid vertical lines mark the respective observed log NISM of the four selected stars.

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