Measuring the ionisation fraction in a jet from a massive protostar

Measuring the ionisation fraction in a jet from a massive protostar

The ionisation fraction of protostellar jets is key to establish their true energetics. Here, the authors determine it in a jet from a high-mass young stellar object, using multi-wavelengths observations, confirming that the ionising mechanism giving rise to the radio emission originates from shocks...

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Autores principales: R. Fedriani, A. Caratti o Garatti, S. J. D. Purser, A. Sanna, J. C. Tan, R. Garcia-Lopez, T. P. Ray, D. Coffey, B. Stecklum, M. Hoare
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2019
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Acceso en línea:https://doaj.org/article/a0e9f0dd86dd4e97a3a2343d442ed8ae
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spelling oai:doaj.org-article:a0e9f0dd86dd4e97a3a2343d442ed8ae2021-12-02T17:01:32ZMeasuring the ionisation fraction in a jet from a massive protostar10.1038/s41467-019-11595-x2041-1723https://doaj.org/article/a0e9f0dd86dd4e97a3a2343d442ed8ae2019-08-01T00:00:00Zhttps://doi.org/10.1038/s41467-019-11595-xhttps://doaj.org/toc/2041-1723The ionisation fraction of protostellar jets is key to establish their true energetics. Here, the authors determine it in a jet from a high-mass young stellar object, using multi-wavelengths observations, confirming that the ionising mechanism giving rise to the radio emission originates from shocks.R. FedrianiA. Caratti o GarattiS. J. D. PurserA. SannaJ. C. TanR. Garcia-LopezT. P. RayD. CoffeyB. StecklumM. HoareNature PortfolioarticleScienceQENNature Communications, Vol 10, Iss 1, Pp 1-9 (2019)
institution DOAJ
collection DOAJ
language EN
topic Science
Q
spellingShingle Science
Q
R. Fedriani
A. Caratti o Garatti
S. J. D. Purser
A. Sanna
J. C. Tan
R. Garcia-Lopez
T. P. Ray
D. Coffey
B. Stecklum
M. Hoare
Measuring the ionisation fraction in a jet from a massive protostar
description The ionisation fraction of protostellar jets is key to establish their true energetics. Here, the authors determine it in a jet from a high-mass young stellar object, using multi-wavelengths observations, confirming that the ionising mechanism giving rise to the radio emission originates from shocks.
format article
author R. Fedriani
A. Caratti o Garatti
S. J. D. Purser
A. Sanna
J. C. Tan
R. Garcia-Lopez
T. P. Ray
D. Coffey
B. Stecklum
M. Hoare
author_facet R. Fedriani
A. Caratti o Garatti
S. J. D. Purser
A. Sanna
J. C. Tan
R. Garcia-Lopez
T. P. Ray
D. Coffey
B. Stecklum
M. Hoare
author_sort R. Fedriani
title Measuring the ionisation fraction in a jet from a massive protostar
title_short Measuring the ionisation fraction in a jet from a massive protostar
title_full Measuring the ionisation fraction in a jet from a massive protostar
title_fullStr Measuring the ionisation fraction in a jet from a massive protostar
title_full_unstemmed Measuring the ionisation fraction in a jet from a massive protostar
title_sort measuring the ionisation fraction in a jet from a massive protostar
publisher Nature Portfolio
publishDate 2019
url https://doaj.org/article/a0e9f0dd86dd4e97a3a2343d442ed8ae
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AT tpray measuringtheionisationfractioninajetfromamassiveprotostar
AT dcoffey measuringtheionisationfractioninajetfromamassiveprotostar
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