activity
20002026
most citedAstrometry of Water Maser Sources in Nearby Molecular Clouds with VERA - II. SVS 13 in NGC 1333

261 citations · 3.3k across the 93 of their papers we have counts for

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31 papers · 1 filter

astro-ph2008★ 7 cited

Microstructure and kinematics of H2O masers in the massive star forming region IRAS 06061+2151

K. Motogi, Y. Watanabe, K. Sorai +14

We have made multi-epoch VLBI observations of H2O maser emission in the massive star forming region IRAS 06061+2151 with the Japanese VLBI network (JVN) from 2005 May to 2007 Octob…

astro-ph2008★ 42 cited

VLBI Astrometry of AGB Variables with VERA -- A Semiregular Variable S Crateris --

Akiharu Nakagawa, Miyuki Tsushima, Kazuma Ando +40

We present a distance measurement for the semiregular variable S Crateris (S Crt) based on its annual parallax. With the unique dual beam system of the VLBI Exploration for Radio A…

astro-ph2008★ 94 cited

Distance to VY Canis Majoris with VERA

Yoon Kyung Choi, Tomoya Hirota, Mareki Honma +33

We report astrometric observations of H2O masers around the red supergiant VY Canis Majoris (VY CMa) carried out with VLBI Exploration of Radio Astrometry (VERA). Based on astromet…

astro-ph2008★ 78 cited

Astrometry of HO Masers in Nearby Star-Forming Regions with VERA. III. IRAS 22198+6336 in L1204G

Tomoya Hirota, Kazuma Ando, Takeshi Bushimata +35

We present results of multi-epoch VLBI observations with VERA (VLBI Exploration of Radio Astrometry) of the 22 GHz HO masers associated with a young stellar object (YSO) IRAS…

astro-ph2008★ 59 cited

Distance to NGC 281 in a Galactic Fragmenting Superbubble: Parallax Measurements with VERA

Mayumi Sato, Tomoya Hirota, Mareki Honma +30

We have used the Japanese VLBI array VERA to perform high-precision astrometry of an H2O maser source in the Galactic star-forming region NGC 281 West, which has been considered to…

astro-ph2008

Molecular Line Observations of the SiO Maser Source IRAS 19312+1950

Jun-ichi Nakashima, Shuji Deguchi, Hiroshi Imai +1

IRAS 19312+1950 is a unique SiO maser source, exhibiting a rich set of molecular radio lines, although SiO maser sources are usually identified as oxygen-rich evolved stars, in whi…