activity
20002023
most citedSpitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

718 citations · 6.4k across the 132 of their papers we have counts for

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17 papers · 1 filter

astro-ph2008

Probing the Galactic cosmic ray flux with submillimeter and gamma ray data

S. Casanova, S. Gabici, F. A. Aharonian +5

The study of Galactic diffuse radiation combined with the knowledge of the distribution of the molecular hydrogen in the Galaxy offers a unique tool to probe the cosmic ray flu…

astro-ph2008★ 14 cited

Catalogue of 12CO(J=1-0) and 13CO(J=1-0) Molecular Clouds in the Carina Flare Supershell

J. R. Dawson, A. Kawamura, N. Mizuno +2

We present a catalogue of 12CO(J=1-0) and 13CO(J=1-0) molecular clouds in the spatio-velocity range of the Carina Flare supershell, GSH 287+04-17. The data cover a region of ~66 sq…

astro-ph2008★ 268 cited

The Second Survey of the Molecular Clouds in the Large Magellanic Cloud by NANTEN I: Catalog of Molecular Clouds

Yasuo Fukui, Akiko Kawamura, Tetsuhiro Minamidani +8

The second survey of the molecular clouds in 12CO (J = 1-0) was carried out in the Large Magellanic Cloud by NANTEN. The sensitivity of this survey is twice as high as that of the…

astro-ph2008★ 25 cited

Aligned Molecular Clouds towards SS433 and L=348.5 degrees; Possible Evidence for Galactic "Vapor Trail" Created by Relativistic Jet

H. Yamamoto, S. Ito, S. Ishigami +8

We have carried out a detailed analysis of the NANTEN 12CO(J=1-0) dataset in two large areas of ~25 square degrees towards SS433 (l~40 degree) and of ~18 square degrees towards l~3…

astro-ph2008★ 36 cited

Submillimeter Line Emission from LMC N159W: a Dense, Clumpy PDR in a Low Metallicity Environment

J. L. Pineda, N. Mizuno, J. Stutzki +30

Star formation at earlier cosmological times takes place in an interstellar medium with low metallicity. The Large Magellanic Cloud (LMC) is ideally suited to study star formation…

astro-ph2008★ 32 cited

The "Carina Flare" Supershell: Probing the Atomic and Molecular ISM in a Galactic Chimney

J. R. Dawson, N. Mizuno, T. Onishi +2

The "Carina Flare" supershell, GSH 287+04-17, is a molecular supershell originally discovered in 12CO(J=1-0) with the NANTEN 4m telescope. We present the first study of the shell's…

astro-ph2007★ 31 cited

12CO 4-3 and [CI] 1-0 at the centers of NGC 4945 and Circinus

M. Hitschfeld, M. Aravena, C. Kramer +30

Studying molecular gas in the central regions of the star burst galaxies NGC4945 and Circinus enables us to characterize the physical conditions and compare them to previous local…

astro-ph2007★ 34 cited

Clumpy photon-dominated regions in Carina. I. [CI] and mid-J CO lines in two 4'x4' fields

C. Kramer, M. Cubick, M. Roellig +31

The Carina region is an excellent astrophysical laboratory for studying the feedback mechanisms of newly born, very massive stars within their natal giant molecular clouds (GMCs) a…

astro-ph2007★ 61 cited

Sub-millimeter Observations of Giant Molecular Clouds in the Large Magellanic Cloud: Temperature and Density as Determined from J=3-2 and J=1-0 transitions of CO

T. Minamidani, N. Mizuno, Y. Mizuno +26

We have carried out sub-mm 12CO(J=3-2) observations of 6 giant molecular clouds (GMCs) in the Large Magellanic Cloud (LMC) with the ASTE 10m sub-mm telescope at a spatial resolutio…

astro-ph2007★ 20 cited

ASTE Submillimeter Observations of a Young Stellar Object Condensation in Cederblad 110

Masaaki Hiramatsu, Takahiro Hayakawa, Ken'ichi Tatematsu +5

We present results of submillimeter observations of a low-mass young stellar objects (YSOs) condensation in the Cederblad 110 region of the Chamaeleon I dark cloud with Atacama Sub…

astro-ph2006★ 201 cited

Spitzer SAGE survey of the Large Magellanic Cloud II: Evolved Stars and Infrared Color Magnitude Diagrams

R. D. Blum, J. R. Mould, K. A. Olsen +47

Color-magnitude diagrams (CMDs) are presented for the Spitzer SAGE (Surveying the Agents of a Galaxy's Evolution) survey of the Large Magellanic Cloud (LMC). IRAC and MIPS 24 um ep…

astro-ph2006★ 718 cited

Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

Margaret Meixner, Karl D. Gordon, Remy Indebetouw +46

We are performing a uniform and unbiased, ~7x7 degrees imaging survey of the Large Magellanic Cloud (LMC), using the IRAC and MIPS instruments on board the Spitzer Space Telescope…

astro-ph2006★ 10 cited

An Observational Perspective of Low Mass Dense Cores II: Evolution towards the Initial Mass Function

D. Ward-Thompson, P. Andre, R. Crutcher +3

We review the properties of low mass dense molecular cloud cores, including starless, prestellar, and Class 0 protostellar cores, as derived from observations. In particular we dis…

astro-ph2006★ 20 cited

Large Scale CO Observations of a Far-Infrared Loop in Pegasus; Detection of a Large Number of Very Small Molecular Clouds Possibly Formed via Shocks

Hiroaki Yamamoto, Akiko Kawamura, Kengo Tachihara +3

We have carried out large scale 12CO and 13CO observations with a mm/sub-mm telescope NANTEN toward a loop-like structure in far infrared whose angular extent is about 20x20 degree…

astro-ph2005★ 26 cited

An Unbiased Survey for Molecular Clouds in the Southern Galactic Warp

Masanori Nakagawa, T. Onishi, A. Mizuno +1

We have made an unbiased survey for molecular clouds in the Galactic Warp. This survey, covering an area of 56 square degrees at l = 252 deg to 266 deg and b = -5 deg to -1 deg, ha…

astro-ph2005★ 99 cited

A Detailed Study of Molecular Clouds toward the TeV Gamma-Ray SNR G347.3-0.5

Y. Moriguchi, K. Tamura, Y. Tawara +4

We present a detailed study of molecular gas toward the supernovae remnant G347.3-0.5 (J1713.7-3946) obtained with the 4m mm/sub-mm telescope NANTEN . This study has revealed that…

astro-ph2000★ 17 cited

Molecular Clouds Around a Run-away O Star, zeta Oph

Kengo Tachihara, Rihei Abe, Toshikazu Onishi +2

Molecular clouds around a run-away O star z Oph have been surveyed with NANTEN telescope and their streaming motion caused by z Oph has been detected. z Oph is the earliest member…