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From the 1 of 153 papers with an AI index.

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20052026
most citedSolar neutrino measurements in Super-Kamiokande-II

445 citations

Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2026

Survival of Molecular Complexity under Recent Supernova Feedback: Detection of Hot Cores in RX J1713.7-3946

Takashi Shimonishi, Hidetoshi Sano, Kenji Furuya +1

Protostellar cores located near supernova remnants are considered potential analogues of the birth environment of the solar system. However, the extent to which supernovae influenc…

astro-ph.GA202520 cited

The Evolutionary Map of the Universe: A new radio atlas for the southern hemisphere sky

A. M. Hopkins, A. Kapinska, J. Marvil +70

We present the Evolutionary Map of the Universe (EMU) survey conducted with the Australian Square Kilometre Array Pathfinder (ASKAP). EMU aims to deliver the touchstone radio atlas…

astro-ph.GA20244 cited

ACA CO(J=2-1) Mapping of the Nearest Spiral Galaxy M33. II. Exploring the Evolution of Giant Molecular Clouds

Ayu Konishi, Kazuyuki Muraoka, Kazuki Tokuda +12

The evolution of giant molecular clouds (GMCs), the main sites of high-mass star formation, is an essential process to unravel the galaxy evolution. Using a GMC catalogue of M33 fr…

astro-ph.GA20241 cited

Sub-kpc scale gas density histogram of the Galactic molecular gas: a new statistical method to characterise galactic-scale gas structures

Ren Matsusaka, Toshihiro Handa, Yusuke Fujimoto +6

To understand physical properties of the interstellar medium (ISM) on various scales, we investigate it at parsec resolution on the kiloparsec scale. Here, we report on the sub-kpc…

astro-ph.GA20171 cited

VLBI Monitoring of the Sub-parsec-scale Jet in the Radio Galaxy 3C 66B at 22 GHz

Hiroshi Sudou, Satoru Iguchi, Guang-Yao Zhao

We present measurements of proper motion of the sub-parsec scale jet at 22 GHz in the nearby FR I galaxy 3C 66B. Observations were made using the VLBA at six epochs over four years…

astro-ph.GA201412 cited

No Microwave Flare of Sagittarius A* around the G2 Periastron Passing

Masato Tsuboi, Yoshiharu Asaki, Osamu Kameya +11

In order to explore any change caused by the G2 cloud approaching, we have monitored the flux density of Sgr A* at 22 GHz from Feb. 2013 to Aug. 2014 with a sub-array of Japanese V…