Figure 7 from The Gould's Belt Very Large Array Survey. I. The Ophiuchus Complex

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The Gould's Belt Very Large Array Survey. I. The Ophiuchus Complex

Authors: Sergio A. Dzib, Laurent Loinard, Amy J. Mioduszewski, Luis F. Rodríguez, Gisela N. Ortiz-León, Gerardo Pech, Juana L. Rivera, Rosa M. Torres, Andrew F. Boden, Lee Hartmann, Neal J. Evans II, Cesar Briceño, and John Tobin

Dzib et al. 2013 The Astrophysical Journal 775 63.

Provider: AAS Journals

Caption: Figure 7.

X-ray luminosity as a function of radio luminosity. The red line corresponds to the Güdel–Benz relation with κ = 1 while the red strip centered on it represents a one order of magnitude dispersion around that relation. The blue line and strip correspond to the Güdel–Benz relation but with κ = 0.03. Colors indicate the evolutionary status of the object as explained at the top left of the diagram.

Other Images in This Article

Copyright and Terms & Conditions