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Non-Thermal Radio Emission from Single Hot Stars
Non-Thermal Radio Emission Single Hot Stars
2009/6/16
Non-Thermal Radio Emission from Single Hot Stars。
Instabilities in Hot Star Winds。
Modeling the Dust and Ammonia Emission in the G 31.41 + 0.31 Hot Molecular Core
G 31.41 + 0.31 Hot Molecular Core Ammonia Emission
2009/6/15
Modeling the Dust and Ammonia Emission in the G 31.41 + 0.31 Hot Molecular Core。
The need for very high resolution spectroscopy for the study of hot subdwarfs
hot subdwarfs spectroscopy
2009/6/11
The need for very high resolution spectroscopy for the study of hot subdwarfs。
The Chemical Evolution of Dynamically Hot Galaxies
Chemical Evolution Dynamically Hot Galaxies
2009/6/5
The Chemical Evolution of Dynamically Hot Galaxies。
Is the plasma within bubbles and superbubbles hot or cold?
Hot gas in the large magellanic cloud。
On determining the sources of hot gas in the halo。
Hot gas and the gaseous structure of the galaxy
HYDRODYNAMICS SUPERNOVAREMNANTS X-RAYS GALAXIES
2009/6/4
A parochial review is presented concerning the status of our understandingof hot gas regions in the Galaxy and their implications for the overall distributionsof the Galaxy抯 gaseous components. We hav...
Needs and requirements for future x-ray observations of hot galactic halos
HALOS X-RAYS JETS AND OUTFLOWS
2009/6/4
Galaxies are key objects for the study of cosmology, the life cycle of matter,and stellar evolution. X-ray observations have given us a new key window intothese building blocks of the Universe, that a...
Major advances have been made in the past decade in our knowledge of the hotinterstellar gas of our Milky Way galaxy. The Di.use X-ray Spectrometer obtainedspectra in the 0.15?.28 keV range from the G...
The Diagnostics of Density Distribution for Dense Hot DT Plasmas Using Fast Protons
Density reconstruction Dense DT plasmas High temperature
2009/6/1
The density reconstruction for dense DT plasmas with high temperature has been studied. In the simulation of a plasma density diagnostics, the energy loss of fast protons going through the plasmas is ...
Necessary conditions for the generation of acoustic solitons in magnetospheric and space plasmas with hot ions
acoustic solitons space plasmas magnetospheric
2009/5/27
Necessary conditions are discussed for the possible generation of large solitary acoustic modes in plasmas with one or more ion species which are hotter than some or all of the electron species. The a...
Spectral Measurements of Cyg X-3: A Thermal Source Embedded in Hot Plasma within a Cold Shell
Low mass X-ray binaries X-ray sources Cyg X-3
2009/5/19
The attempts at unified model fitting to explain the spectral
variations in Cyg X-3 suggest equally probable fits with a combination of
an absorbed blackbody and a separately absorbed power law with...
Physics of the Sun’s Hot Atmosphere
Solar X-ray and EUV emission coronal heating solar wind
2009/5/7
This article briefly overviews the physics of the Sun`s hot atmosphere,using observations from recent solar spacecrafts: Yohkoh, SOHO, TRACE and RHESSI.