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Large-scale structure of the molecular gas in Taurus revealed by high linear dynamic range spectral line mapping
molecules structure
2014/12/23
We report the results of a 100 deg2 survey of the Taurus molecular cloud region in 12CO and 13CO J = 1→ 0. The image of the cloud in each velocity channel includes 3 × 106 Nyquist-sampled pixels on a ...
S0 galaxies are often thought to be passively evolved from spirals after star formation is quenched. To explore what is actually occurring in such galaxies, we present a multi-wavelength case study of...
Surveying the Dynamic Radio Sky with the Long Wavelength Demonstrator Array
the Dynamic Radio Sky the Long Wavelength Demonstrator Array
2011/1/13
This paper presents a search for radio transients at a frequency of 73.8 MHz (4 m wavelength) using the all-sky imaging capabilities of the Long Wavelength Demonstrator Array (LWDA). The LWDA was a 16...
Observing and modeling the dynamic atmosphere of the low mass-loss C-star R Sculptoris at high angular resolution
Solar and Stellar Astrophysics (astro-ph.SR)
2010/12/27
We study the circumstellar environment of the carbon-rich star R Scl using the near- and mid-infrared high spatial resolution observations from the ESO-VLTI instruments VINCI and MIDI. These observati...
Dynamic Shocks in the Inhomogeneous Environment of the Cygnus Loop
Inhomogeneous Environment Cygnus Loop
2009/6/16
Dynamic Shocks in the Inhomogeneous Environment of the Cygnus Loop。
RADAR TIME DELAYS IN THE DYNAMIC THEORY OF GRAVITY
Gravitation-Relativity-Methods analytical-Techiques radar astronomy
2009/3/6
There is a new theory gravity called the dynamic theory, which is
derived from thermodynamic principles in a five dimensional space, radar signals
travelling times and delays are calculated for the ...