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DISTANCE DETERMINATION TO THE CRAB-LIKE PULSAR WIND NEBULA G54.1+0.3 AND THE SEARCH FOR ITS SUPERNOVA REMNANT SHELL
supernova remnants molecules radio continuum
2014/12/23
We discovered a large-scale shell G53.9+0.2 around the Crab-like pulsar wind nebula (PWN) G54.1+0.3 with 1420 MHz continuum Very Large Array observations. This is confirmed by a new infrared (IR) imag...
Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
neutron stars gravitational waves cosmology
2011/10/14
Detection of gravitational waves from the inspiral phase of binary neutron star coalescence will allow us to measure the effects of the tidal coupling in such systems. These effects will be measurable...
Why the Fundamental Plane of Black Hole Activity is not a Distance Artifact
Fundamental Plane Distance Artifact Black Hole Activity
2009/7/1
Why the Fundamental Plane of Black Hole Activity is not a Distance Artifact。
Relation between a Function of the Right Ascension and the Angular Distance to the Vertex for Hyades Stars
Moving clusters Hyades cluster open clusters Hyades astrometric and kinematic
2009/5/14
In this paper, relation was developed for Hyades stars between
a function of the right ascensions and the angular distances from the vertex.
The precision criteria of this relation are very satisfac...
DISTANCE TO THE ORIGEM AND THE MONOCEROS LOOPS
THE ORIGEM THE MONOCEROS LOOPS Supernova Remnants
2009/3/26
Using the Supernova Remnants (SNR) hypothesis for the radio
loops, distances of the Origem and the Monoceros loops were calculated from the
surface brightness and the angular diameters at 1420 MHz. ...