Star Formation Laws in Both Galactic Massive Clumps and External Galaxies: Extensive Study with Dust Coninuum, HCN (4-3), and CS (7-6) - INSU - Institut national des sciences de l'Univers Accéder directement au contenu
Article Dans Une Revue The Astrophysical Journal Année : 2016

Star Formation Laws in Both Galactic Massive Clumps and External Galaxies: Extensive Study with Dust Coninuum, HCN (4-3), and CS (7-6)

Tie Liu
  • Fonction : Auteur
Kee-Tae Kim
Hyunju Yoo
  • Fonction : Auteur
Sheng-Yuan Liu
  • Fonction : Auteur
Ken'Ichi Tatematsu
  • Fonction : Auteur
Sheng-Li Qin
  • Fonction : Auteur
Qizhou Zhang
Yuefang Wu
  • Fonction : Auteur
Ke Wang
Paul F. Goldsmith
  • Fonction : Auteur
Mika Juvela
  • Fonction : Auteur
Jeong-Eun Lee
  • Fonction : Auteur
L. Viktor Tóth
  • Fonction : Auteur
Diego Mardones
  • Fonction : Auteur
Guido Garay
  • Fonction : Auteur
Leonardo Bronfman
  • Fonction : Auteur
Maria R. Cunningham
  • Fonction : Auteur
Di Li
  • Fonction : Auteur
Nadia Lo
  • Fonction : Auteur
Scott Schnee
  • Fonction : Auteur

Résumé

We observed 146 Galactic clumps in HCN (4-3) and CS (7-6) with the Atacama Submillimeter Telescope Experiment 10 m telescope. A tight linear relationship between star formation rate and gas mass traced by dust continuum emission was found for both Galactic clumps and the high redshift (z > 1) star forming galaxies (SFGs), indicating a constant gas depletion time of ∼100 Myr for molecular gas in both Galactic clumps and high z SFGs. However, low z galaxies do not follow this relation and seem to have a longer global gas depletion time. The correlations between total infrared luminosities (L TIR) and molecular line luminosities ({L}{mol}\prime ) of HCN (4-3) and CS (7-6) are tight and sublinear extending down to clumps with L TIR ∼ 103 L . These correlations become linear when extended to external galaxies. A bimodal behavior in the L TIR-{L}{mol}\prime correlations was found for clumps with different dust temperature, luminosity-to-mass ratio, and σ linevir. Such bimodal behavior may be due to evolutionary effects. The slopes of L TIR-L‧mol correlations become more shallow as clumps evolve. We compared our results with lower J transition lines in Wu et al. (2010). The correlations between clump masses and line luminosities are close to linear for low effective excitation density tracers but become sublinear for high effective excitation density tracers for clumps with L TIR larger than L TIR ∼ 104.5 L . High effective excitation density tracers cannot linearly trace the total clump masses, leading to a sublinear correlations for both M clump-L‧mol and L TIR-L‧mol relations.

Dates et versions

insu-03669428 , version 1 (16-05-2022)

Identifiants

Citer

Tie Liu, Kee-Tae Kim, Hyunju Yoo, Sheng-Yuan Liu, Ken'Ichi Tatematsu, et al.. Star Formation Laws in Both Galactic Massive Clumps and External Galaxies: Extensive Study with Dust Coninuum, HCN (4-3), and CS (7-6). The Astrophysical Journal, 2016, 829, ⟨10.3847/0004-637X/829/2/59⟩. ⟨insu-03669428⟩
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