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Hatsukade, B., Tamura, Y., Iono, D., Matsuda, Y., Hayashi, M. and Oguri, M. (2015) High-Resolution ALMA Observations of SDP. 81. II. Molecular Clump Properties of a Lensed Submillimeter Galaxy at z = 3.042. Publications of the Astronomical Society of Japan, 67, 93.
https://doi.org/10.1093/pasj/psv061

has been cited by the following article:

• TITLE: The Giants Arcs as Modeled by the Superbubbles

  AUTHORS: Lorenzo Zaninetti

  KEYWORDS: Galaxy Groups, Clusters and Superclusters, Large Scale Structure of the Universe Cosmology

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.5 No.2, April 8, 2019

  ABSTRACT: The giant arcs in the clusters of galaxies are modeled in the framework of the superbubbles. The density of the intracluster medium is assumed to follow a hyperbolic behavior. The analytical law of motion is function of the elapsed time and the polar angle. As a consequence the flux of kinetic energy in the expanding thin layer decreases with increasing polar angle making the giant arc invisible to the astronomical observations. In order to calibrate the arcsec-parsec conversion three cosmologies are analyzed.