Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5

Kosuke Fujii; Tetsuhiro Minamidani; N. Mizuno; T. Onishi; A. Kawamura; Erik Muller; Joanne Dawson; Y. Fukui

Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5

Kosuke Fujii, Tetsuhiro Minamidani, N. Mizuno, T. Onishi, A. Kawamura, Erik Muller, Joanne Dawson, Y. Fukui

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution

Abstract

The (CO)-C-12(J=3-2/1-0) and (CO)-C-13(T=3-2/1-0) observations with ASTE and Mopra telescopes have been carried out toward the giant molecular clouds (GMCs) in the N48/N49 regions in the Large Magellanic Cloud (LMC), which are located at the boundary of two kpc-scale Supergiant Shell (SGS) LMC 4 & LMC 5. The star formation is relatively evolved in the N48 region, which is just located at the boundary of SGSs, than in the N49 region. The clumps in the N48 show higher n(H-2) and T-kin than those in the N49, but their densities are not so high as the LMC cluster forming clumps. The collision of two SGSs actually enhances the star formation but further evolution seem to be necessary for subsequent cluster formation.

Original language	English
Title of host publication	Revolution in astronomy with ALMA
Subtitle of host publication	the third year: proceedings of a conference held at the Tokyo International Forum, Tokyo, Japan, 8-11 December 2014
Editors	Daisuke Iono, Ken'ichi Tatematsu, Alwyn Wootten, Leonardo Testi
Place of Publication	San Francisco
Publisher	Astronomical Society of the Pacific
Pages	255-256
Number of pages	2
ISBN (Electronic)	1583818839, 9781583818831
ISBN (Print)	9781583818824, 1583818820
Publication status	Published - 2015
Event	4th ALMA Science Conference on Revolution in Astronomy with ALMA: The Third Year - Tokyo, Japan Duration: 8 Dec 2014 → 11 Dec 2014

Publication series

Name	Astronomical Society of the Pacific Conference Series
Publisher	Astronomical Society of the Pacific
Volume	499
ISSN (Print)	1050-3390

Conference

Conference	4th ALMA Science Conference on Revolution in Astronomy with ALMA: The Third Year
Country/Territory	Japan
City	Tokyo
Period	8/12/14 → 11/12/14

Keywords

LARGE-MAGELLANIC-CLOUD
GIANT
TEMPERATURE

Cite this

Fujii, K., Minamidani, T., Mizuno, N., Onishi, T., Kawamura, A., Muller, E., Dawson, J., & Fukui, Y. (2015). Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5. In D. Iono, K. Tatematsu, A. Wootten, & L. Testi (Eds.), Revolution in astronomy with ALMA: the third year: proceedings of a conference held at the Tokyo International Forum, Tokyo, Japan, 8-11 December 2014 (pp. 255-256). (Astronomical Society of the Pacific Conference Series; Vol. 499). Astronomical Society of the Pacific.

Fujii, Kosuke ; Minamidani, Tetsuhiro ; Mizuno, N. et al. / Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5. Revolution in astronomy with ALMA: the third year: proceedings of a conference held at the Tokyo International Forum, Tokyo, Japan, 8-11 December 2014. editor / Daisuke Iono ; Ken'ichi Tatematsu ; Alwyn Wootten ; Leonardo Testi. San Francisco : Astronomical Society of the Pacific, 2015. pp. 255-256 (Astronomical Society of the Pacific Conference Series).

@inproceedings{af43c2c1664e48e3a6d78011c5c31dc3,

title = "Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5",

abstract = "The (CO)-C-12(J=3-2/1-0) and (CO)-C-13(T=3-2/1-0) observations with ASTE and Mopra telescopes have been carried out toward the giant molecular clouds (GMCs) in the N48/N49 regions in the Large Magellanic Cloud (LMC), which are located at the boundary of two kpc-scale Supergiant Shell (SGS) LMC 4 & LMC 5. The star formation is relatively evolved in the N48 region, which is just located at the boundary of SGSs, than in the N49 region. The clumps in the N48 show higher n(H-2) and T-kin than those in the N49, but their densities are not so high as the LMC cluster forming clumps. The collision of two SGSs actually enhances the star formation but further evolution seem to be necessary for subsequent cluster formation.",

keywords = "LARGE-MAGELLANIC-CLOUD, GIANT, TEMPERATURE",

author = "Kosuke Fujii and Tetsuhiro Minamidani and N. Mizuno and T. Onishi and A. Kawamura and Erik Muller and Joanne Dawson and Y. Fukui",

year = "2015",

language = "English",

isbn = "9781583818824",

series = "Astronomical Society of the Pacific Conference Series",

publisher = "Astronomical Society of the Pacific",

pages = "255--256",

editor = "Daisuke Iono and Ken'ichi Tatematsu and Alwyn Wootten and Leonardo Testi",

booktitle = "Revolution in astronomy with ALMA",

note = "4th ALMA Science Conference on Revolution in Astronomy with ALMA: The Third Year ; Conference date: 08-12-2014 Through 11-12-2014",

}

Fujii, K, Minamidani, T, Mizuno, N, Onishi, T, Kawamura, A, Muller, E, Dawson, J & Fukui, Y 2015, Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5. in D Iono, K Tatematsu, A Wootten & L Testi (eds), Revolution in astronomy with ALMA: the third year: proceedings of a conference held at the Tokyo International Forum, Tokyo, Japan, 8-11 December 2014. Astronomical Society of the Pacific Conference Series, vol. 499, Astronomical Society of the Pacific, San Francisco, pp. 255-256, 4th ALMA Science Conference on Revolution in Astronomy with ALMA: The Third Year, Tokyo, Japan, 8/12/14.

Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5. / Fujii, Kosuke; Minamidani, Tetsuhiro; Mizuno, N. et al.
Revolution in astronomy with ALMA: the third year: proceedings of a conference held at the Tokyo International Forum, Tokyo, Japan, 8-11 December 2014. ed. / Daisuke Iono; Ken'ichi Tatematsu; Alwyn Wootten; Leonardo Testi. San Francisco: Astronomical Society of the Pacific, 2015. p. 255-256 (Astronomical Society of the Pacific Conference Series; Vol. 499).

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution

TY - GEN

T1 - Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5

AU - Fujii, Kosuke

AU - Minamidani, Tetsuhiro

AU - Mizuno, N.

AU - Onishi, T.

AU - Kawamura, A.

AU - Muller, Erik

AU - Dawson, Joanne

AU - Fukui, Y.

PY - 2015

Y1 - 2015

N2 - The (CO)-C-12(J=3-2/1-0) and (CO)-C-13(T=3-2/1-0) observations with ASTE and Mopra telescopes have been carried out toward the giant molecular clouds (GMCs) in the N48/N49 regions in the Large Magellanic Cloud (LMC), which are located at the boundary of two kpc-scale Supergiant Shell (SGS) LMC 4 & LMC 5. The star formation is relatively evolved in the N48 region, which is just located at the boundary of SGSs, than in the N49 region. The clumps in the N48 show higher n(H-2) and T-kin than those in the N49, but their densities are not so high as the LMC cluster forming clumps. The collision of two SGSs actually enhances the star formation but further evolution seem to be necessary for subsequent cluster formation.

AB - The (CO)-C-12(J=3-2/1-0) and (CO)-C-13(T=3-2/1-0) observations with ASTE and Mopra telescopes have been carried out toward the giant molecular clouds (GMCs) in the N48/N49 regions in the Large Magellanic Cloud (LMC), which are located at the boundary of two kpc-scale Supergiant Shell (SGS) LMC 4 & LMC 5. The star formation is relatively evolved in the N48 region, which is just located at the boundary of SGSs, than in the N49 region. The clumps in the N48 show higher n(H-2) and T-kin than those in the N49, but their densities are not so high as the LMC cluster forming clumps. The collision of two SGSs actually enhances the star formation but further evolution seem to be necessary for subsequent cluster formation.

KW - LARGE-MAGELLANIC-CLOUD

KW - GIANT

KW - TEMPERATURE

M3 - Conference proceeding contribution

SN - 9781583818824

SN - 1583818820

T3 - Astronomical Society of the Pacific Conference Series

SP - 255

EP - 256

BT - Revolution in astronomy with ALMA

A2 - Iono, Daisuke

A2 - Tatematsu, Ken'ichi

A2 - Wootten, Alwyn

A2 - Testi, Leonardo

PB - Astronomical Society of the Pacific

CY - San Francisco

T2 - 4th ALMA Science Conference on Revolution in Astronomy with ALMA: The Third Year

Y2 - 8 December 2014 through 11 December 2014

ER -

Fujii K, Minamidani T, Mizuno N, Onishi T, Kawamura A, Muller E et al. Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5. In Iono D, Tatematsu K, Wootten A, Testi L, editors, Revolution in astronomy with ALMA: the third year: proceedings of a conference held at the Tokyo International Forum, Tokyo, Japan, 8-11 December 2014. San Francisco: Astronomical Society of the Pacific. 2015. p. 255-256. (Astronomical Society of the Pacific Conference Series).

Dense molecular clumps associated with the LMC supergiant shell LMC 4 & LMC 5

Abstract

Publication series

Conference

Keywords

Fingerprint

Cite this