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20112026
most citedMolecular Clouds Toward the Super Star Cluster NGC3603; Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation

164 citations · 845 across the 17 of their papers we have counts for

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11 papers · 1 filter

astro-ph.GA2026

Deep HI observations of cold gas inflow and outflow

W. J. G. de Blok, D. B. Fisher, K. Tachihara +8

A major question in galaxy evolution is how galaxies acquire sufficient gas to sustain their star formation rates. HI observations with high angular resolution and sensitivity to v…

astro-ph.GA2025

Head-tail molecular clouds falling onto the Milky Way disk

Mikito Kohno, Yasuo Fukui, Takahiro Hayakawa +13

We report discovery of two CO clouds which are likely falling down to the Galactic plane at more than km s. The clouds show head-tail distributions elongated perpendicu…

astro-ph.GA2023★ 6 cited

Giant molecular clouds and their Type classification in M74: Toward understanding star formation and cloud evolution

F. Demachi, Y. Fukui, R. I. Yamada +10

We investigated the giant molecular clouds (GMCs) in M74 (NGC 628), using data obtained from the PHANGS project. We applied the GMC Types according to the activity of star formatio…

astro-ph.GA2014★ 27 cited

A Young GMC Formed at the Interface of Two Colliding Supershells: Observations Meet Simulations

J. R. Dawson, E. Ntormousi, Y. Fukui +2

Dense, star-forming gas is believed to form at the stagnation points of large-scale ISM flows, but observational examples of this process in action are rare. We here present a gian…

astro-ph.GA2014★ 26 cited

Characterizing the structure of diffuse emission in Hi-GAL maps

D. Elia, F. Strafella, N. Schneider +18

We present a study of the structure of the Galactic interstellar medium through the Delta-variance technique, related to the power spectrum and the fractal properties of infrared/s…

astro-ph.GA2014★ 81 cited

Optically thick HI dominant in the local interstellar medium; an alternative interpretation to "dark gas"

Y. Fukui, K. Torii, T. Onishi +5

Dark gas in the interstellar medium (ISM) is believed to not be detectable either in CO or Hi radio emission, but it is detected by other means including gamma-rays, dust emission…

astro-ph.GA2013★ 49 cited

SPLASH: The Southern Parkes Large-Area Survey in Hydroxyl - First Science from the Pilot Region

J. R. Dawson, A. J. Walsh, P. A. Jones +20

SPLASH (the Southern Parkes Large-Area Survey in Hydroxyl) is a sensitive, unbiased and fully-sampled survey of the Southern Galactic Plane and Galactic Centre in all four ground-s…

astro-ph.GA2013★ 164 cited

Molecular Clouds Toward the Super Star Cluster NGC3603; Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation

Yasuo Fukui, Akio Ohama, Naoki Hanaoka +17

We present new large field observations of molecular clouds with NANTEN2 toward the super star cluster NGC3603 in the transitions 12CO(J=2-1, J=1-0) and 13CO(J=2-1, J=1-0). We sugg…

astro-ph.GA2013★ 119 cited

The first Hi-GAL observations of the outer Galaxy: a look to star formation in the third Galactic quadrant in the longitude range 216.5 < l < 225.5

D. Elia, S. Molinari, Y. Fukui +17

We present the first Herschel PACS and SPIRE photometric observations in a portion of the outer Galaxy ( and $-2^{\circ} \lesssi…

astro-ph.GA2013★ 55 cited

Non-thermal X-rays and interstellar gas toward the γ-ray supernova remnant RX J1713.7-3946: Evidence for X-ray enhancement around CO and HI clumps

H. Sano, T. Tanaka, K. Torii +18

RX J1713.7-3946 is the most remarkable very-high-energy γ-ray supernova remnant which emits synchrotron X-rays without thermal features. We made a comparative study of CO, HI and X…

astro-ph.GA2011★ 139 cited

A Detailed Study of the Molecular and Atomic Gas Toward the γ-ray SNR RX J1713.7-3946: Spatial TeV γ-ray and ISM Gas Correspondence

Y. Fukui, H. Sano, J. Sato +14

RX J1713.73946 is the most remarkable TeV -ray SNR which emits -rays in the highest energy range. We made a new combined analysis of CO and \ion{H}{1} in the SNR and deriv…