Evidence for recent star formation in BCGs: a correspondence between blue cores and UV excess |
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| Authors: | A Pipino S Kaviraj C Bildfell A Babul H Hoekstra † J Silk |
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| Institution: | Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH;Department of Physics and Astronomy, University of Southern California, Los Angeles 90089-0740, USA;Department of Physics and Astronomy, University of Victoria, Victoria, BC V8P 1A1, Canada;Sterrewacht Leiden, Leiden University, Niels Bohrweg 2, NL-2333 CA Leiden, the Netherlands |
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| Abstract: | We present a joint analysis of near-ultraviolet ( NUV ) data from the GALEX ( Galaxy Evolution Explorer ) mission and (optical) colour profiles for a sample of seven brightest cluster galaxies (BCGs) in the Canadian Cluster Comparison Project. We find that every BCG, which has a blue rest-frame UV colour, also shows a blue core in its optical colour profile. Conversely, BCGs that lack blue cores and show monotonic colour gradients typical of old elliptical galaxies are red in the UV. We interpret this as evidence that the NUV enhancement in the blue BCGs is driven by recent star formation and not from old evolved stellar populations such as horizontal branch stars. Furthermore, the UV enhancement cannot be from an active galactic nuclei (AGN) because the spatial extent of the blue cores is significantly larger than the possible contamination region due to a massive black hole. The recent star formation in the blue BCGs typically has an age less than 200 Myr and contributes mass fractions of less than a per cent. Although the sample studied here is small, we demonstrate, for the first time , a one-to-one correspondence between blue cores in elliptical galaxies (in particular BCGs) and a NUV enhancement observed using GALEX . The combination of this one-to-one correspondence and the consistently young age of recent star formation, coupled with additional correlations with the host cluster's X-ray properties, strongly suggests that the star formation is fuelled by gas cooling out of the intracluster medium. In turn, this implies that any AGN heating of the intracluster medium in massive clusters only acts to reduce the magnitude of the cooling flow and once this flow starts, it is nearly always active. Collectively, these results suggest that AGN feedback in present-day BCGs, while important, cannot be as efficient as suggested by the recent theoretical model by proposed by De Lucia et al. |
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| Keywords: | galaxies: clusters: general cooling flows galaxies: elliptical and lenticular cD galaxies: evolution X-rays: galaxies: clusters |
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