output
19972026
most citedHI4PI: A full-sky HI survey based on EBHIS and GASS

1.6k citations

Showing 2015 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2015★ 22 cited

Unusual shock-excited OH maser emission in a young Planetary Nebula

Hai-Hua Qiao, Andrew J. Walsh, Jose F. Gomez +9

We report on OH maser emission toward G336.644-0.695 (IRAS 16333-4807), which is a H2O maser-emitting Planetary Nebula (PN). We have detected 1612, 1667 and 1720 MHz OH masers at t…

astro-ph.GA2015★ 133 cited

Three-Dimensional Distribution of the ISM in the Milky Way Galaxy: III. The Total Neutral Gas Disk

Hiroyuki Nakanishi, Yoshiaki Sofue

We present newly obtained three-dimensional gaseous maps of the Milky Way Galaxy; HI, H and total-gas (HI plus H) maps, which were derived from the HI and CO(--…

astro-ph.GA2015★ 63 cited

A precessing molecular jet signaling an obscured, growing supermassive black hole in NGC1377?

S. Aalto, F. Costagliola, S. Muller +11

With high resolution (0."25 x 0."18) ALMA CO 3-2 observations of the nearby (D=21 Mpc, 1"=102 pc), extremely radio-quiet galaxy NGC1377, we have discovered a high-velocity, very co…

astro-ph.GA2015★ 74 cited

Obscuring Fraction of Active Galactic Nuclei: Implications from Radiation-driven Fountain Models

Keiichi Wada

Active galactic nuclei (AGNs) are believed to be obscured by an optical thick "torus" that covers a large fraction of solid angles for the nuclei. However, the physical origin of t…

astro-ph.GA2015★ 26 cited

Concurrent Formation of Carbon and Silicate Dust in Nova V1280 Sco

Itsuki Sakon, Shigeyuki Sako, Takashi Onaka +12

We present infrared multi-epoch observations of the dust forming nova V1280 Sco over 2000 days from the outburst. The temporal evolution of the infrared spectral energy distr…

astro-ph.GA2015

Outer Rotation Curve of the Galaxy with VERA III: Astrometry of IRAS 07427-2400 and Test of the Density-Wave Theory

Nobuyuki Sakai, Hiroyuki Nakanishi, Mitsuhiro Matsuo +6

We report the trigonometric parallax of IRAS 07427-2400 with VERA to be 0.185 0.027 mas, corresponding to a distance of 5.41 kpc. The result is consistent w…