activity
19982023
most citedExtragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)

690 citations · 13.3k across the 204 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

11 papers · 2 filters

astro-ph2005★ 257 cited

A size of ~1 AU for the radio source Sgr A* at the centre of the Milky Way

Zhi-Qiang Shen, K. Y. Lo, M. -C. Liang +2

Although it is widely accepted that most galaxies have supermassive black holes (SMBHs) at their centers^{1-3}, concrete proof has proved elusive. Sagittarius A* (Sgr A*)^4, an ext…

astro-ph2005★ 71 cited

Submillimeter emission from the hot molecular jet HH 211

A. Palau, P. T. P. Ho, Q. Zhang +7

We observed the HH 211 jet in the submillimeter continuum and the CO(3-2) and SiO(8-7) transitions with the Submillimeter Array. The continuum source detected at the center of the…

astro-ph2005★ 105 cited

SiO J=5--4 in the HH211 Protostellar Jet Imaged with the SMA

Naomi Hirano, Sheng-Yuan Liu, Hsien Shang +5

We have mapped the SiO J=5-4 line at 217GHz from the HH211 molecular outflow with the Submillimeter Array (SMA). The high resolution map (1.6''x0.9'') shows that the SiO J=5-4 emis…

astro-ph2005★ 97 cited

CO J=6-5 observations of TW Hya with the SMA

C. Qi, D. J. Wilner, N. Calvet +5

We present the first images of the 691.473 GHz CO J=6-5 line in a protoplanetary disk, obtained along with the 690 GHz dust continuum, toward the classical T Tauri star TW Hya usin…

astro-ph2005★ 72 cited

Infall and Outflow around the HH 212 protostellar system

Chin-Fei Lee, Paul T. P. Ho, Henrik Beuther +4

HH 212 is a highly collimated jet discovered in H2 powered by a young Class 0 source, IRAS 05413-0104, in the L1630 cloud of Orion. We have mapped around it in 1.33 mm continuum, 1…

astro-ph2005★ 202 cited

A disk of dust and molecular gas around a high-mass protostar

Nimesh A. Patel, Salvador Curiel, T. K. Sridharan +7

The processes leading to the birth of low-mass stars such as our Sun have been well studied, but the formation of high-mass (> 8 x Sun's mass) stars has heretofore remained poorly…

astro-ph2005★ 120 cited

Submm line imaging of Orion-KL with the Submillimeter Array

H. Beuther, Q. Zhang, L. J. Greenhill +8

We present the first submm (865mum) imaging spectral line survey at one arcsecond resolution conducted with the Submillimeter Array toward Orion-KL. Within the 2x2 GHz bandpasses (…

astro-ph2005★ 31 cited

An Infalling Torus of Molecular Gas Around the Ultra-Compact HII Region G28.20-0.05

Peter K. Sollins, Qizhou Zhang, Eric Keto +1

We present new observations of the ultra-compact HII region G28.20-0.05 in 23 GHz continuum, and the NH3(1,1), NH3(2.2), and NH3(3,3) lines. To explain the complicated kinematics o…

astro-ph2005★ 53 cited

The Molecular Accretion Flow in G10.6-0.4

Peter K. Sollins, Paul T. P Ho

We have observed the ultracompact HII region G10.6-0.4 with the VLA in 23 GHz continuum and the NH3(3,3) inversion line. By analyzing the optical depth of the line as well as the k…

astro-ph2005★ 72 cited

IRAS 16293-2442B: A Compact, Possibly Isolated Protoplanetary Disk in a Class 0 Object

Luis F. Rodriguez, Laurent Loinard, Paola D'Alessio +2

Theoretical arguments suggest that protoplanetary disks around young stars should start small and grow with the addition of high angular momentum material to reach the radii of sev…

astro-ph2005★ 52 cited

Atomic and Molecular Gas in Colliding Galaxy Systems: I. The Data

Daisuke Iono, Min S. Yun, Paul T. P. Ho

We present HI and CO(1-0) interferometric observations of 10 comparable-mass interacting systems obtained at the Very Large Array (VLA) and the Owens Valley Radio Observatory (OVRO…