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19972011
most citedTrigonometric Parallaxes of Massive Star Forming Regions: V. G23.01-0.41 and G23.44-0.18

105 citations · 237 across the 8 of their papers we have counts for

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astro-ph2008105 cited

Trigonometric Parallaxes of Massive Star Forming Regions: V. G23.01-0.41 and G23.44-0.18

A. Brunthaler, M. J. Reid, K. M. Menten +3

We report trigonometric parallaxes for the massive star-forming regions G23.01-0.41 and G23.44-0.18, corresponding to distances of 4.59 [+0.38/-0.33] kpc and 5.88 [+1.37/-0.93] kpc…

astro-ph20086 cited

Scaling Relation between Sunyaev-Zel'dovich Effect and X-ray Luminosity and Scale-Free Evolution of Cosmic Baryon Field

Qiang Yuan, Hao-Yi Wan, Tong-Jie Zhang +3

It has been revealed recently that, in the scale free range, i.e. from the scale of the onset of nonlinear evolution to the scale of dissipation, the velocity and mass density fiel…

astro-ph200873 cited

The RMS Survey: CO observations of candidate massive YSOs in the northern Galactic plane

J. S. Urquhart, A. L. Busfield, M. G. Hoare +9

Context: The Red MSX Source (RMS) survey is an ongoing multi-wavelength observational programme designed to return a large, high-resolution mid-infrared colour-selected sample of m…

astro-ph200731 cited

The interstellar medium of the Antennae Galaxies

A. Schulz, C. Henkel, D. Muders +3

To study the properties of the interstellar medium in the prototypical merging system of the Antennae galaxies (NGC 4038 and NGC 4039), we have obtained CO(1-0), (2-1) and (3-2) li…

astro-ph200613 cited

A WENO Algorithm of the Temperature and Ionization Profiles around a Point Source

Jing-Mei Qiu, Long-Long Feng, Chi-Wang Shu +1

We develop a numerical solver for radiative transfer problems based on the weighted essentially nonoscillatory (WENO) scheme modified with anti-diffusive flux corrections, in order…

astro-ph2003

Effects of dark-matter density profiles on bulge formation in very late-type galaxies

Jie-Hao Huang, Zu-Gan Deng, Yan-Ning Fu

The dynamical evolution of super star clusters has been investigated in dark matter halos depicted with a cuspy- or soft-core density profile. The simulations show that (1) exponen…