activity
20022022
most citedNeutral pion emission from accelerated protons in the supernova remnant W44

229 citations · 4.1k across the 95 of their papers we have counts for

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Showing 2014 · astro-ph.GAShow all

4 papers · 2 filters

astro-ph.GA2014★ 97 cited

Mapping the Milky Way bulge at high resolution: the 3D dust extinction, CO, and X factor maps

M. Schultheis, B. Q. Chen, B. W. Jiang +6

Three dimensional interstellar extinction maps provide a powerful tool for stellar population analysis. We use data from the VISTA Variables in the Via Lactea survey together with…

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.GA2014★ 11 cited

The jet and arc molecular clouds toward Westerlund 2, RCW 49, and HESS J1023-575; 12CO and 13CO (J=2-1 and J=1-0) observations with NANTEN2 and Mopra Telescope

N. Furukawa, A. Ohama, T. Fukuda +20

We have made new CO observations of two molecular clouds, which we call "jet" and "arc" clouds, toward the stellar cluster Westerlund 2 and the TeV gamma-ray source HESS J1023-575.…

astro-ph.GA2014★ 57 cited

HI, CO, and Planck/IRAS dust properties in the high-latitude-cloud complex, MBM 53, 54, 55 and HLCG 92-35; Possible evidence for an optically thick HI envelope around the CO clouds

Yasuo Fukui, Ryuji Okamoto, Ryohei Kaji +9

We present an analysis of the HI and CO gas in conjunction with the Planck/IRAS submillimeter/far-infrared dust properties toward the most outstanding high latitude clouds MBM 53,…