Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Rodón, Javier A."'
Autor:
Figueira, Miguel, Bronfman, Leonardo, Zavagno, Annie, Louvet, Fabien, Lo, Nadia, Finger, Ricardo, Rodón, Javier
Publikováno v:
A&A 616, L10 (2018)
Little is known about how high-mass stars form. Around 30\% of the young high-mass stars in the Galaxy are observed at the edges of ionized (HII) regions. Therefore these are places of choice to study the earliest stages of high-mass star formation,
Externí odkaz:
http://arxiv.org/abs/1807.11860
FU Orionis stars (FUORS) are eruptive pre-main sequence objects thought to represent quasi-periodic or recurring stages of enhanced accretion during the low-mass star-forming process. We characterize the sample of known and candidate FUORS in an homo
Externí odkaz:
http://arxiv.org/abs/1402.3240
Autor:
Wang, Yuan, Beuther, Henrik, Zhang, Qizhou, Bik, Arjan, Rodon, Javier A., Jiang, Zhibo, Fallscheer, Cassandra
We observed three high-mass star-forming regions in the W3 high-mass star formation complex with the Submillimeter Array and IRAM 30 m telescope. These regions, i.e. W3 SMS1 (W3 IRS5), SMS2 (W3 IRS4) and SMS3, are in different evolutionary stages and
Externí odkaz:
http://arxiv.org/abs/1205.5333
Autor:
Figueira, Miguel, Bronfman, Leonardo, Zavagno, Annie, Louvet, Fabien, Lo, Nadia, Finger, Ricardo, Rodón, Javier
Publikováno v:
XXXIX Polish Astronomical Society Meeting
XXXIX Polish Astronomical Society Meeting, 2019, Olsztyn, Poland. pp.142-146
XXXIX Polish Astronomical Society Meeting, 2019, Olsztyn, Poland. pp.142-146
International audience; High-mass stars are primordial objects in the study of star formation since their feedback has a significant impact on the interstellar medium. The budget of momentum and energy of feedback can change the properties of the new
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4b81e4477c23803edfebb1233ad64155
https://amu.hal.science/hal-03561801
https://amu.hal.science/hal-03561801
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
FU Orionis stars (FUors) are eruptive pre-main sequence objects thought to represent quasi-periodic or recurring stages of enhanced accretion during the low-mass star-forming process. We characterize the sample of known and candidate FUors in a homog
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::eaeb3dc014422e0014e186b433cef30d
http://iopscience.iop.org/article/10.1088/0004-6256/147/6/140/meta
http://iopscience.iop.org/article/10.1088/0004-6256/147/6/140/meta
Autor:
Rodón, Javier Adrián
Since its discovery by E. Salpeter in 1955, the high-mass end of the Initial Mass Function (IMF) has been continuously tested, and its slope has not changed from the value -2.35 originally calculated by Salpeter, the "Salpeter value". Furthermore, it
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f567198b73f5e54920b3ec407cb8bffb
http://archiv.ub.uni-heidelberg.de/volltextserver/10037/
http://archiv.ub.uni-heidelberg.de/volltextserver/10037/
Akademický článek
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Publikováno v:
Labyrinth of Star Formation; 2014, p425-427, 3p
Autor:
Wang, Yuan, Beuther, Henrik, Zhang, Qizhou, Bik, Arjan, Rodón, Javier A., Jiang, Zhibo, Fallscheer, Cassandra
Publikováno v:
Proceedings of the International Astronomical Union; Aug2012 Supplement, Vol. 8 Issue S292, p116-116, 1p