Abstract
Abstract
We report on a nearly factor-of-ten fade and then re-brightening after several months of [CMD97]-1031, a candidate young stellar object. Through fitting of light curve data from ZTF and ATLAS, we find a dip amplitude >2.5 mag and duration 80–320 days. After the large dip, the source recovered to slightly fainter brightness and redder color.
Publisher
American Astronomical Society
Cited by
1 articles.
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