<p>HCG 16 is a rare (very compact) group of galaxies made of solely spiral galaxies showing diffuse X-ray emission. The figure shows optical (greyscale from the Digitized Sky Survey) and X-ray (contours, Chandra ACIS-S3, ObsID 923, PI Mamon) views of HCG 16. Chandra chip is 8 arcmin across. The four luminous galaxies are (left to right) NGC 839 (HCG 16d), NGC 838 (HCG 16c), NGC 835 (HCG 16a) and NGC 833 (HCG 16b). The Chandra contours are for the energy band 0.4–1.57 keV. This unpublished image was corrected for the exposure map in 4 energy bands, and processed with CIAO 2.2.1 in March 2002. </p
Contributions to the XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society, held 13...
Aims. We investigate the X-ray properties of four isolated elliptical galaxies, selected from the Up...
Restricted Access. An open-access version is available at arXiv.org. Articles older than 2 years are...
13 pages, 6 figures, uses aa.cls style, Latex.We report results obtained from analysis of the XMM-Ne...
We present new, deep Chandra X-ray and Giant Metrewave Radio Telescope 610 MHz observations of the s...
International audienceWe present new, deep Chandra X-ray and Giant Metrewave Radio Telescope 610 MHz...
We use a combination of deep Chandra X-ray observations and radio continuum imaging to investigate t...
International audienceWe use a combination of deep Chandra X-ray observations and radio continuum im...
International audienceGalaxy groups provide the environment in which the majority of galaxies evolve...
We present an analysis of the diffuse X-ray emission in 19 compact groups of galaxies (CGs) observed...
We present follow-up optical g', r', and i' imaging and spectroscopy of serendipitous X-ray sources ...
We present high-resolution X-ray imaging data from the ACIS-S instrument on the Chandra telescope of...
We searched the public archive of the Chandra X-ray Observatory as of 2016 March and assembled a sam...
A Chandra X-Ray Observatory ACIS-S imaging observation is used to study the population of X-ray sour...
Color poster with text, images, and charts (Spring 2009)We have obtained X-ray data from the orbitin...
Contributions to the XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society, held 13...
Aims. We investigate the X-ray properties of four isolated elliptical galaxies, selected from the Up...
Restricted Access. An open-access version is available at arXiv.org. Articles older than 2 years are...
13 pages, 6 figures, uses aa.cls style, Latex.We report results obtained from analysis of the XMM-Ne...
We present new, deep Chandra X-ray and Giant Metrewave Radio Telescope 610 MHz observations of the s...
International audienceWe present new, deep Chandra X-ray and Giant Metrewave Radio Telescope 610 MHz...
We use a combination of deep Chandra X-ray observations and radio continuum imaging to investigate t...
International audienceWe use a combination of deep Chandra X-ray observations and radio continuum im...
International audienceGalaxy groups provide the environment in which the majority of galaxies evolve...
We present an analysis of the diffuse X-ray emission in 19 compact groups of galaxies (CGs) observed...
We present follow-up optical g', r', and i' imaging and spectroscopy of serendipitous X-ray sources ...
We present high-resolution X-ray imaging data from the ACIS-S instrument on the Chandra telescope of...
We searched the public archive of the Chandra X-ray Observatory as of 2016 March and assembled a sam...
A Chandra X-Ray Observatory ACIS-S imaging observation is used to study the population of X-ray sour...
Color poster with text, images, and charts (Spring 2009)We have obtained X-ray data from the orbitin...
Contributions to the XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society, held 13...
Aims. We investigate the X-ray properties of four isolated elliptical galaxies, selected from the Up...
Restricted Access. An open-access version is available at arXiv.org. Articles older than 2 years are...