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Filamentary accretion flows in high-mass star-forming clouds
by
Beltran, M T
, Cesaroni, R
, Beuther, H
, Feng, S
, Palau, A
, J -E Schneider
, Wells, M R A
, Klessen, R
, Jiao, S
, Leurini, S
, Klaassen, P
, Gieser, C
, Urquhart, J S
, Pudritz, R
in
Continuum radiation
/ Gas flow
/ Massive stars
/ Star formation
2025
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Filamentary accretion flows in high-mass star-forming clouds
by
Beltran, M T
, Cesaroni, R
, Beuther, H
, Feng, S
, Palau, A
, J -E Schneider
, Wells, M R A
, Klessen, R
, Jiao, S
, Leurini, S
, Klaassen, P
, Gieser, C
, Urquhart, J S
, Pudritz, R
in
Continuum radiation
/ Gas flow
/ Massive stars
/ Star formation
2025
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Do you wish to request the book?
Filamentary accretion flows in high-mass star-forming clouds
by
Beltran, M T
, Cesaroni, R
, Beuther, H
, Feng, S
, Palau, A
, J -E Schneider
, Wells, M R A
, Klessen, R
, Jiao, S
, Leurini, S
, Klaassen, P
, Gieser, C
, Urquhart, J S
, Pudritz, R
in
Continuum radiation
/ Gas flow
/ Massive stars
/ Star formation
2025
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Filamentary accretion flows in high-mass star-forming clouds
Paper
Filamentary accretion flows in high-mass star-forming clouds
2025
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Overview
We quantify the gas flows from a scale of up to several parsecs down to the sub-parsec scale along filamentary structures in the three high-mass star-forming regions G75.78, IRAS21078+5211 and NGC7538 with data obtained from the IRAM 30 m telescope. The analysis is carried out using the surface density derived from 1.2 mm continuum emission and velocity differences estimated from HCO\\(^+\\) and H\\(^13\\)CO\\(^+\\) molecular line data.
Publisher
Cornell University Library, arXiv.org
Subject
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