We present the mid-infrared star formation rates of 245 X-ray selected, nearby (z < 0.1) brightest cluster galaxies (BCGs). A homogeneous and volume limited sample of BCGs was created by X-ray selecting clusters with Lx > 1 × 1044 erg s⁻ ¹. The Wide-Field Infrared Survey Explorer (WISE) All WISE Data Release provides the first measurement of the 12 μm star formation indicator for all BCGs in the nearby Universe. Perseus A and Cygnus A are the only galaxies in our sample to have star formation rates of > 40 M⊙ yr⁻¹, indicating that these two galaxies are highly unusual at current times. Stellar populations of 99 ± 0.6 per cent of local BCGs are (approximately) passively evolving, with star formation rates of < 10 M⊙ yr⁻¹. We find that ...
Brightest Cluster Galaxies (BCGs) are typically massive ellipticals at the centers of clusters. They...
We study the properties of brightest cluster galaxies (BCGs) drawn from a catalogue of more than 69 ...
We examine the role of environment on the in situ star formation (SF) hosted by the progenitors of t...
We investigate the near-infrared evolution of brightest cluster galaxies (BCGs) from a sample of ric...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of a Spitzer/Herschel infrared photometric analysis of the largest (716) and ...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of a Spitzer/Herschel infrared photometric analysis of the largest (716) and ...
We present a study of the evolution of brightest cluster galaxies (BCGs) in a sample of clusters at ...
We present a study of the evolution of brightest cluster galaxies (BCGs) in a sample of clusters at ...
We present a study of the evolution of brightest cluster galaxies (BCGs) in a sample of clusters at ...
Brightest Cluster Galaxies (BCGs) are typically massive ellipticals at the centers of clusters. The...
We present a sample of 329 low to intermediate redshift ($0.05 < z < 0.3$) brightest cluster galaxie...
Brightest Cluster Galaxies (BCGs) are typically massive ellipticals at the centers of clusters. They...
We study the properties of brightest cluster galaxies (BCGs) drawn from a catalogue of more than 69 ...
We examine the role of environment on the in situ star formation (SF) hosted by the progenitors of t...
We investigate the near-infrared evolution of brightest cluster galaxies (BCGs) from a sample of ric...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of a Spitzer/Herschel infrared photometric analysis of the largest (716) and ...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of an MIPS-24 μm study of the brightest cluster galaxies (BCGs) of 535 high-r...
We present the results of a Spitzer/Herschel infrared photometric analysis of the largest (716) and ...
We present a study of the evolution of brightest cluster galaxies (BCGs) in a sample of clusters at ...
We present a study of the evolution of brightest cluster galaxies (BCGs) in a sample of clusters at ...
We present a study of the evolution of brightest cluster galaxies (BCGs) in a sample of clusters at ...
Brightest Cluster Galaxies (BCGs) are typically massive ellipticals at the centers of clusters. The...
We present a sample of 329 low to intermediate redshift ($0.05 < z < 0.3$) brightest cluster galaxie...
Brightest Cluster Galaxies (BCGs) are typically massive ellipticals at the centers of clusters. They...
We study the properties of brightest cluster galaxies (BCGs) drawn from a catalogue of more than 69 ...
We examine the role of environment on the in situ star formation (SF) hosted by the progenitors of t...