The Nature of the Variable Galactic Center Source IRS16SW
classification
🌌 astro-ph
keywords
variablesourcecentercurvegalacticirs16swlightbinary
read the original abstract
We report measurements of the light curve of the variable Galactic Center source IRS16SW. The light curve is not consistent with an eclipsing binary or any other obvious variable star. The source may be an example of a high mass variable predicted theoretically but not observed previously.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.