Results 41 to 50 of about 2,697 (212)
Published as part of Kime, Richard Desmond & Enghoff, Henrik, 2017, Atlas of European millipedes 2: Order Julida (Class Diplopoda), pp. 1-299 in European Journal of Taxonomy 346 on page 69, DOI: 10.5852/ejt.2017.346, http://zenodo.org/record ...
Kime, Richard Desmond, Enghoff, Henrik
openaire +2 more sources
Multiwavelength VLBI observations of Sagittarius A* [PDF]
14pages, 14 Figures, Accepted for publication in A& ...
Sabine König+12 more
openaire +3 more sources
Testing alternative theories of gravity by fitting the hot-spot data of Sgr A*
We are fitting dynamics of electrically neutral hot-spot orbiting around Sagittarius A* (Sgr A*) source in Galactic center, represented by various modifications of the standard Kerr black hole (BH), to the three flares observed by the GRAVITY instrument ...
Misbah Shahzadi+3 more
doaj +1 more source
GALACTIC CENTER MINISPIRAL: INTERACTION MODES OF NEUTRON STARS
Streams of gas and dust in the inner parsec of the Galactic center form a distinct feature known as the Minispiral, which has been studied in radio waveband as well as in the infrared wavebands.
Michal Zajacek+2 more
doaj +1 more source
Precession of timelike bound orbits in Kerr spacetime
Astrometric observations of S-stars provide a unique opportunity to probe the nature of Sagittarius-A* (Sgr-A*). In view of this, it has become important to understand the nature and behavior of timelike bound trajectories of particles around a massive ...
Parth Bambhaniya+5 more
doaj +1 more source
The Variability of Sagittarius A* at Centimeter Wavelengths
We present the results of a 3.3-year project to monitor the flux density of Sagittarius A* at 2.0, 1.3, and 0.7 cm with the VLA. The fully calibrated light curves for Sgr A* at all three wavelengths are presented. Typical errors in the flux density are 6.1%, 6.2%, and 9.2% at 2.0, 1.3, and 0.7 cm, respectively.
Jun-Hui Zhao+3 more
openaire +4 more sources
We develop a new method for studying the Galactic magnetic field along the spiral arms using pulsar Faraday rotation measures (RMs). Our new technique accounts for the dot-product nature of Faraday rotation and also splits the associated path integral ...
Alice P. Curtin+2 more
doaj +1 more source
The Multifrequency Behavior of Sagittarius A* [PDF]
The Galactic Center is the closest galactic nucleus that allows us to determine the multi-frequency behavior of the supermassive black hole counterpart Sagittarius A* in great detail. We put SgrA*, as a nucleus with weak activity, into the context of nearby low luminosity nuclei.
Nastaran Fazeli+16 more
openaire +3 more sources
On the Structure of the Sagittarius Spiral Arm in the Inner Milky Way
We report measurements of trigonometric parallax and proper motion for two 6.7 GHz methanol and two 22 GHz water masers located in the far portion of the Sagittarius spiral arm as part of the BeSSeL Survey.
S. B. Bian+8 more
doaj +1 more source
THE INTRINSIC TWO-DIMENSIONAL SIZE OF SAGITTARIUS A* [PDF]
accepted for publication in ...
Mark Morris+16 more
openaire +6 more sources