Long-term study of water maser emission associated with Young Stellar Objects. II: Analysis

Autor: Brand J. 1, Cesaroni R. 2, Comoretto G. 2, Felli M. 2, Palagi F. 1, Palla F. 2, Valdettaro R. 2

Publikováno v: 407 (2003): 573.
info:cnr-pdr/source/autori:Brand J. 1, Cesaroni R. 2, Comoretto G. 2, Felli M. 2, Palagi F. 1, Palla F. 2, Valdettaro R. 2/titolo:Long-term study of water maser emission associated with Young Stellar Objects. II: Analysis/doi:/rivista:/anno:2003/pagina_da:573/pagina_a:/intervallo_pagine:573/volume:407

We present the analysis of the properties of water maser emission in 14 star forming regions (SFRs), which have been monitored for up to 13 years with a sampling rate of about once every 2-3 months. The 14 regions were chosen to span a range in lumin

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=cnr_________::8e517742eda6cdd3b1c3fd6e55d1dbc4
https://publications.cnr.it/doc/5890