Short- and long-term variability of young stars in the Orion Nebula Cluster and Molecular Cloud
V. M. Rivilla, C. J. Chandler, J. Sanz-Forcada, I. Jim\'enez-Serra, J., Forbrich, J. Mart\'in-Pintado

TL;DR
This study used multi-epoch radio observations to analyze variability in young stars within the Orion Nebula Cluster, revealing frequent radio flares and their potential link to X-ray activity, thus advancing understanding of stellar magnetic phenomena.
Contribution
First multi-epoch radio monitoring of Orion young stars, identifying frequent radio flares and their correlation with X-ray activity, providing new insights into stellar magnetic processes.
Findings
Detected 19 radio sources with variability in most epochs.
First detection of radio flares in OHC-E.
Estimated radio flaring rate of 0.14 flares per day.
Abstract
We used the Very Large Array to carry out a multi-epoch radio continuum monitoring of the Orion Nebula Cluster and Orion Molecular Cloud. Our observations reveal the presence of 19 sources. With the exception of the sources BN and C the sources show variability between the different epochs. We have found tentative evidence of variability in the massive object related with source I. Our observations also confirm radio flux density variations of a factor >2 on timescales of hours to days in 5 sources. One of these flaring sources, OHC-E, has been detected for the first time. We conclude that the radio emission arises from: i) highly-variable non-thermal gyrosynchrotron emission produced by electrons accelerated in the magnetospheres of pre-main sequence stars; ii) thermal emission from ionized gas and/or heated dust around massive objects and proplyds. Combining our sample with other…
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