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- W2964473103 abstract "In this study we analyze 70 radio continuum sources that are associated with dust clumps and which are considered to be candidates for the earliest stages of high-mass star formation. The detection of these sources was reported by Rosero et al., who found most of them to show weak ( mJy) and compact ( 06) radio emission. Herein, we used the observed parameters of these sources to investigate the origin of the radio continuum emission. We found that at least ∼30% of these radio detections are most likely to be ionized jets associated with high-mass protostars. However, for the most compact sources, we cannot discard the scenario that they represent pressure-confined H ii regions. This result is highly relevant for recent theoretical models that are based on core accretion, which predict the first stages of ionization from high-mass stars to be in the form of jets. Additionally, we found that properties such as the radio luminosity as a function of the bolometric luminosity of ionized jets from low and high-mass stars are extremely well-correlated. Our data improve upon previous studies by providing further evidence of a common origin for jets independently of luminosity." @default.
- W2964473103 created "2019-08-13" @default.
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- W2964473103 date "2019-07-30" @default.
- W2964473103 modified "2023-10-17" @default.
- W2964473103 title "Weak and Compact Radio Emission in Early High-mass Star-forming Regions. II. The Nature of the Radio Sources" @default.
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