Search for new water vapor masers in the direction of ROW 19-20, 38 and 48-49

Details Search for new water vapor masers in the direction of ROW 19-20, 38 and 48-49 Search for new water vapor masers in the direction of ROW 19-20, 38 and 48-49

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ipespreptq....d&link_type=abstract

M.S. Thesis - 26 Aug. 1983 Instituto de Pesquisas Espaciais, Sao Jose dos Campos (Brazil).

Other

Masers, Stars, Stellar Evolution, Water Vapor, Gravitational Fields, Hydrodynamic Equations, Isothermal Processes, Shock Fronts, Spatial Distribution

Scientific paper

The identification of regions of sequential massive star formation, using maser sources of H2O molecule as indicators is discussed. The equations that govern the evolution of a shock front produced by the ionizing radiation of an OB star group are derived. The stability conditions in this shock front are then analyzed. The binomial H2O maser-massiver star is examined to clarify why regions of recent star formation are being identified using maser sources. From the three choosen regions, RCW 19-20, RCW 38 and RCW 48-49, only RCW 38 shows the necessary conditions for the above identification.

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