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搜索结果: 1-13 共查到理学 radio emission相关记录13条 . 查询时间(0.114 秒)
We analyzed new 237 MHz and 614 MHz GMRT data of the most X-ray luminous galaxy cluster, RX J1347-1145. Our radio results are compared with the MUSTANG 90 GHz Sunyaev-Zel'dovich effect map and with re...
We investigate the conditions for radio emission in rotating and oscillating magnetars, by focusing on the main physical processes determining the position of their death-lines in the P-\dot{P} diagra...
We present the evolutionary properties and luminosity functions of the radio sources belonging to the Chandra Deep Field South VLA survey, which reaches a flux density limit at 1.4 GHz of 43 microJy a...
We present multi-epoch radio and optical observations of the M7 dwarf 2MASS J13142039+1320011. We detect a ~1 mJy source at 1.43, 4.86, 8.46 and 22.5 GHz, making it the most luminous radio emission ov...
Synchrotron radio emission in radio-quiet AGNs     Synchrotron radio emission  radio-quiet AGNs       font style='font-size:12px;'> 2011/1/11
The basic mechanism responsible for radio emission in radio-loud active galactic nuclei (AGNs) is assumed to be synchrotron radiation. We suggest here that radio emission in radio-quiet objects is als...
In recent years, the freely available Monte Carlo code REAS for modelling radio emission from cosmic ray air showers has evolved to include the full complexity of air shower physics. However, it turne...
Compact radio emission in Ultra Luminous X-ray sources      Galaxies  general – X-rays  general – ISM  HII regions       font style='font-size:12px;'> 2010/11/10
We present results from our studies of radio emission from selectecd Ultra Luminous X-ray (ULX) sources, using archival Giant Metrewave Radio Telescope (GMRT) data and new European VLBI Network (EVN) ...
Radio emission from the massive stars in Westerlund 1      Radio emission  massive stars in Westerlund 1        font style='font-size:12px;'> 2010/11/10
The diverse massive stellar population in the young massive clusterWesterlund 1 (Wd 1)provides an ideal laboratory to observe and constrain mass-loss processes throughout the transitional phase of mas...
We report the discovery made using the Australia Telescope Compact Array of a remarkable string of radio emission towards IRAS 16562-3959, a luminous infrared source with a bolometric luminosity of $7...
The 8 o'clock arc is a gravitationally lensed Lyman Break Galaxy (LBG) at redshift z=2.73 that has a star-formation rate (SFR) of 270 solar-mass/year (derived from optical and near-infrared spectrosco...
Non-Thermal Radio Emission from Single Hot Stars     Non-Thermal Radio Emission  Single Hot Stars       font style='font-size:12px;'> 2009/6/16
Non-Thermal Radio Emission from Single Hot Stars
Radio emission models of Colliding-Wind Binaries     Radio emission models  Colliding-Wind Binaries       font style='font-size:12px;'> 2009/6/15
Radio emission models of Colliding-Wind Binaries
Gamma-ray and VLBI Radio Emission from Gamma-ray-loud Blazars           font style='font-size:12px;'> 2007/7/28
期刊信息 篇名 Gamma-ray and VLBI Radio Emission from Gamma-ray-loud Blazars 语种 英文 撰写或编译 撰写 作者 Dai Benzhong,Xie Guangzhong,Mei Dongcheng 第一作者单位 云南大学物理系 刊物名称 Astrophysics and Space Science 页面 287-296 出版日期 200...

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