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Browsing University of Hertfordshire by Author "Rivilla, V. M."
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The feedback of an HC H II region on its parental molecular core : The case of core A1 in the star-forming region G24.78+0.08
Moscadelli, L.; Rivilla, V. M.; Cesaroni, R.; Beltrán, M. T.; Sánchez-Monge, A.; Schilke, P.; Mottram, J. C.; Ahmadi, A.; Allen, V.; Beuther, H.; Csengeri, T.; Etoka, S.; Galli, D.; Goddi, C.; Johnston, K. G.; Klaassen, P. D.; Kuiper, R.; Kumar, M. S.N.; Maud, L. T.; Möller, T.; Peters, T.; Van Der Tak, F.; Vig, S. (2018-08-01)Context. G24.78+0.08 is a well known high-mass star-forming region, where several molecular cores harboring OB young stellar objects are found inside a clump of size 1 pc. This article focuses on the most prominent of these ... -
Short- and long-term variability of young stars in the Orion Nebula Cluster and Molecular Cloud
Rivilla, V. M.; Chandler, C. J.; Sanz-Forcada, J.; Jiménez-Serra, I.; Forbrich, J.; Martín-Pintado, J. (2015-04-03)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 ... -
A systematic survey of millimetre-wavelength flaring variability of Young Stellar Objects in the Orion Nebula Cluster
Vargas-González, J.; Forbrich, J.; Rivilla, V. M.; Menten, K. M.; Güdel, M.; Hacar, A. (2023-03-29)High-energy processes are ubiquitous even in the earliest stages of protostellar evolution. Motivated by the results of our systematic search for intense centimeter radio flares in Young Stellar Objects (YSOs) and by rare ...