Researchers from the Kavli Institute for Particle Astrophysics and Cosmology (KIPAC), jointly run by Stanford University and the Department of Energy's SLAC National Accelerator Laboratory, shed light on this important era by analyzing 84 sets of
X-ray telescope observations from the Japanese - US Suzaku satellite.
Not exact matches
Soon after the initial
observations of the merger site, the Earth's annual trip around the Sun placed the object too close to the Sun in the sky for
X-ray and visible - light
telescopes to observe.
«Various
observations of one particular star over the years and with different
telescopes have revealed vastly different things — at one time a pulsar and the other an
X-ray binary,» said Alessandro Papitto of the Institute of Space Sciences (Consejo Superior de Investigaciones Cientificas — Institut d'Estudis Espacials de Catalunya) in Barcelona, Spain, and lead author of a paper published in the journal Nature.
Heinz and his colleagues quickly mounted a series of follow - up
observations with the space - based Chandra and XMM - Newton
telescopes to discover four bright rings of
X-rays, like ripples in a cosmic pond, all around the neutron star at the heart of Circinus X-1.
Additional
observations and archival data from other
telescopes confirmed the on - again, off - again cycle of
X-ray and radio pulsations.
The first two disks zoom into the central galaxy cluster, the third disk (far right) demonstrates how an
observation of the zoom area would look with an
X-ray telescope («virtual
telescope»).
To determine just how far away they are, researchers will combine the information from the Hubble images with
observations taken by NASA's Spitzer and Chandra space
telescopes, which see in infrared and
x-ray light, respectively.
This is important for other radio, optical,
X-ray and gamma - ray
telescopes so they can follow up
observations of these cosmic events with their own
observation.
To study the process, Brickhouse and her team combined
observations from NASA's Chandra
X-ray Observatory with those from ground - based optical
telescopes.
But
observations beginning in 2014 from NASA's NuSTAR and other space
telescopes are showing that some ULXs, which glow with
X-ray light equal in energy to millions of suns, are actually neutron stars — the burnt - out cores of massive stars that exploded.
Science Interests Formation of galaxies and black holes in the early universe and their growth over cosmic time; large surveys with Hubble and other
telescopes to discover new populations of distant galaxies and black holes; physical properties of active galactic nuclei using
observations from radio, infrared, optical, ultraviolet through to
X-ray energies.
The European
X-ray Observatory Satellite (EXOSAT), originally named HELOS, was an
X-ray telescope operational from May 1983 until April 1986 and in that time made 1780
observations in the
X-ray band of most classes of astronomical object including active galactic nuclei, stellar coronae, cataclysmic variables, white dwarfs,
X-ray binaries, clusters of galaxies, and supernova remnants.