{ "id": "1204.3808", "version": "v1", "published": "2012-04-17T14:56:52.000Z", "updated": "2012-04-17T14:56:52.000Z", "title": "Water maser kinematics in massive star-forming regions: Cepheus A and W75N", "authors": [ "J. M. Torrelles", "N. A. Patel", "S. Curiel", "J. F. Gómez", "G. Anglada", "R. Estalella" ], "comment": "Submitted to Bolet\\'in de la Asociaci\\'on Argentina de Astronom\\'ia (BAAA), Vol. 54, AAA-SOCHIAS meeting (September 17-21, 2011)", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "VLBI multi-epoch water maser observations are a powerful tool to study the dense, warm shocked gas very close to massive protostars. The very high-angular resolution of these observations allow us to measure the proper motions of the masers in a few weeks, and together with the radial velocity, to determine their full kinematics. In this paper we present a summary of the main observational results obtained toward the massive star-forming regions of Cepheus A and W75N, among them: (i) the identification of different centers of high-mass star formation activity at scales of 100 AU; (ii) the discovery of new phenomena associated with the early stages of high-mass protostellar evolution (e.g., isotropic gas ejections); and (iii) the identification of the simultaneous presence of a wide-angle outflow and a highly collimated jet in the massive object Cep A HW2, similar to what is observed in some low-mass protostars. Some of the implications of these results in the study of high-mass star formation are discussed.", "revisions": [ { "version": "v1", "updated": "2012-04-17T14:56:52.000Z" } ], "analyses": { "keywords": [ "massive star-forming regions", "water maser kinematics", "vlbi multi-epoch water maser observations", "high-mass star formation activity" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1111115, "adsabs": "2012arXiv1204.3808T" } } }