[HTML][HTML] Water maser variability in a high-mass YSO outburst-VERA and ALMA observations of S255 NIRS 3

T Hirota, R Cesaroni, L Moscadelli, K Sugiyama… - Astronomy & …, 2021 - aanda.org
Context. Clarifying the relationship between mass accretion and ejection history is one of the
key issues in understanding high-mass star formation processes. Aims. We aim to …

Water maser variability in a high-mass YSO outburst

T Hirota, R Cesaroni, L Moscadelli, K Sugiyama… - Astronomy & …, 2021 - cir.nii.ac.jp
抄録< jats: p>< jats: italic> Context.</jats: italic> Clarifying the relationship between mass
accretion and ejection history is one of the key issues in understanding high-mass star …

Water maser variability in a high-mass YSO outburst. VERA and ALMA observations of S255 NIRS 3

T Hirota, R CESARONI, L MOSCADELLI, K Sugiyama… - 2021 - openaccess.inaf.it
Context. Clarifying the relationship between mass accretion and ejection history is one of the
key issues in understanding high-mass star formation processes. Aims: We aim to …

Water maser variability in a high-mass YSO outburst--VERA and ALMA observations of S255 NIRS 3

T Hirota, R Cesaroni, L Moscadelli, K Sugiyama… - arXiv preprint arXiv …, 2020 - arxiv.org
We carried out observations of the 22 GHz H2O masers in a high-mass protostar S255 NIRS
3 by using VERA. We measured the proper motions of the 22 GHz H2O masers associated …

Water maser variability in a high-mass YSO outburst. VERA and ALMA observations of S255 NIRS 3

T Hirota, R Cesaroni, L Moscadelli… - Astronomy and …, 2021 - ui.adsabs.harvard.edu
Context. Clarifying the relationship between mass accretion and ejection history is one of the
key issues in understanding high-mass star formation processes. Aims: We aim to …

Water maser variability in a high-mass YSO outburst. VERA and ALMA observations of S255 NIRS 3

T Hirota, R Cesaroni, L Moscadelli… - Astronomy and …, 2021 - ui.adsabs.harvard.edu
Context. Clarifying the relationship between mass accretion and ejection history is one of the
key issues in understanding high-mass star formation processes. Aims: We aim to …