Extending theLX–Trelation from clusters to groups

2014/10/20 by V. Bharadwaj, T. H. Reiprich, L. Lovisari +1 · 2 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics #Bolometer #Computer science #Data mining #Galaxies: Formation, Evolution, Phenomena #Galaxy #Optics #Physics #Pulsars and Gravitational Waves Research #Relation (database) #Selection (genetic algorithm) #astro-ph.CO #astro-ph.HE

paper · pdf · doi:10.1051/0004-6361/201424586

published as A&A 573, A75 (2015) · Accepted for publication in Astronomy and Astrophysics

arxiv created 2014/10/20 · openalex publication_date 2014/11/05 · arxiv updated 2014/12/24 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We aim to investigate the bolometric LX − T relation for galaxy groups, and to study the impact of gas cooling, feedback from super-massive black holes, and the selection effects on it.

Citations

• The Evolution of X‐Ray Clusters in a Low‐Density Universe
• The X-ray virial relations for relaxed lensing clusters observed withChandra
• CHANDRACLUSTER COSMOLOGY PROJECT. II. SAMPLES AND X-RAY DATA REDUCTION
• Simulations of AGN Feedback in Galaxy Clusters and Groups: Impact on Gas Fractions and the L X - T Scaling Relation
• The Two Micron All Sky Survey (2MASS)
• Toward a Halo Mass Function for Precision Cosmology: The Limits of Universality

Cited by

• Cosmological implications of the anisotropy of ten galaxy cluster scaling relations
• SEMI-ANALYTIC GALAXY EVOLUTION (SAGE): MODEL CALIBRATION AND BASIC RESULTS