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A rare and persistent rapid-fire fast radio burst source – sending out an occasional and informative cosmic ping from more than 3.5 billion light years away – now helps to reveal the secrets of the br...
What seemed a cosmic trickle almost a decade ago now appears as a rapid-fire barrage from across the universe.
Precise Location,Distance Provide Breakthrough in Study of Fast Radio Bursts
Precise Location Distance Breakthrough Fast Radio Bursts
2017/1/9
For the first time, astronomers have pinpointed the location in the sky of a Fast Radio Burst (FRB), allowing them to determine the distance and home galaxy of one of these mysterious pulses of radio ...
The International Centre for Radio Astronomy Research（ICRAR）
The International Centre for Radio Astronomy Research ICRAR
2014/6/23
The International Centre for Radio Astronomy Research is a collaborative centre that is international in scope and that achieves research excellence in astronomical science and engineering.
F-GAMMA: On the phenomenological classification of continuum radio spectra variability patterns of Fermi blazars
F-GAMMA phenomenological classification continuum radio spectra variability patterns Fermi blazars
2012/2/21
The F-GAMMA program is a coordinated effort to investigate the physics of Active Galactic Nuclei (AGNs) via multi-frequency monitoring of Fermi blazars. In the current study we show and discuss the ev...
Explaining radio emission of magnetars via rotating and oscillating magnetospheres of neutron stars
MHD: pulsars — general — relativity — oscillations — magnetar — stars:neutron — death line — plasma magnetosphere
2011/10/10
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...
Unveiling the nature of IGR J17177-3656 with X-ray, NIR and Radio observations
Unveiling IGR J17177-3656 X-ray NIR Radio observations
2011/9/26
We report on the first broad-band (1-200 keV) simultaneous Chandra-INTEGRAL observations of the recently discovered hard X-ray transient IGR J17177-3656 that took place on 2011, March 22, about two we...
Electron Temperatures in W51 Complex from High Resolution, Low Frequency Radio Observations
ISM—HII regions—radio continuum—individual (W51)
2010/9/15
W51 is a giant radio complex lying along the tangent to the Sagitarius arm at a distance of about 7 kpc from the Sun, with an extension of about 1◦ in the sky. It is divided into three component...
Large scale absorbers in the environment of high-z radio-galaxies。
VLA Detection of a Double Radio Source at the Center of the HH 288 Quadrupolar Outflow
VLA HH 288 Quadrupolar Outflow Double Radio
2009/6/16
VLA Detection of a Double Radio Source at the Center of the HH 288 Quadrupolar Outflow。
The emission line regions of redshift one radio galaxies
emission line regions redshift radio galaxies
2009/6/10
The emission line regions of redshift one radio galaxies。
Observations of radio galaxy mrc 1138-262: merging galaxies embedded in a giant Lya halo
radio galaxy Lya halo
2009/6/10
Observations of radio galaxy mrc 1138-262：merging galaxies embedded in a giant Lya halo。
Evidence for jet-cloud interactions in high-redshift radio galaxies
jet-cloud interactions high-redshift radio galaxies
2009/6/10
Evidence for jet-cloud interactions in high-redshift radio galaxies。
Detection, Excision and Statistics of Interference at the Mauritius Radio Telescope
Metre-wave radio telescope Fourier synthesis interference excision
2009/5/20
A technique to detect man-made interference in the visibility
data of the Mauritius Radio Telescope (MRT) has been developed. This
technique is based on the understanding that the interference is ge...
A POSITION CATALOGUE OF 146 HLS STARS AND 78 RADIO STARS OBSERVED WITH THE BELGRADE MERIDIAN CIRCLE
146 HLS STARS BELGRADE MERIDIAN CIRCLE 78 RADIO STARS
2009/4/8
The authors present an observational catalogue containing the positions
of 146 high-luminosity stars, as well as the optical counterparts of 78 radio
stars worked out by diffrential method in the FK...