Quenching cluster cooling flows with recurrent hot plasma bubbles
(2004)
Journal Article
Dalla Vecchia, C., Bower, R., Theuns, T., Balogh, M., Mazzotta, P., & Frenk, C. (2004). Quenching cluster cooling flows with recurrent hot plasma bubbles. Monthly Notices of the Royal Astronomical Society, 355, 995-1004. https://doi.org/10.1111/j.1365-2966.2004.08381.x
Outputs (4)
The second-generation VLT instrument MUSE: science drivers and instrument design (2004)
Presentation / Conference Contribution
Bacon, R., Bauer, S.-M., Bower, R., Cabrit, S., Cappellari, M., Carollo, M., Combes, F., Davies, R. L., Delabre, B., Dekker, H., Devriendt, J., Djidel, S., Duchateau, M., Dubois, J.-P., Emsellem, E., Ferruit, P., Franx, M., Gilmore, G. F., Guiderdoni, B., Henault, F., …de Zeeuw, P. T. (2004, December). The second-generation VLT instrument MUSE: science drivers and instrument design
Deep SAURON spectral imaging of the diffuse Lyman α halo LAB1 in SSA 22. (2004)
Journal Article
Bower, R., Morris, S., Bacon, R., Wilman, R., Sullivan, M., Chapman, S., …Emsellem, E. (2004). Deep SAURON spectral imaging of the diffuse Lyman α halo LAB1 in SSA 22. Monthly Notices of the Royal Astronomical Society, 351(1), 63-69. https://doi.org/10.1111/j.1365-2966.2004.07783.xWe have used the SAURON panoramic integral field spectrograph to study the structure of the Lyα emission-line halo, LAB1, surrounding the submillimetre galaxy SMM J221726+0013. This emission-line halo was discovered during a narrow-band imaging surve... Read More about Deep SAURON spectral imaging of the diffuse Lyman α halo LAB1 in SSA 22..
Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS (2004)
Journal Article
Baugh, C., Bower, R., Cole, S., Eke, V., Baldry, I., Balogh, M., …Taylor, K. (2004). Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS. Monthly Notices of the Royal Astronomical Society, 348(4), 1355-1372. https://doi.org/10.1111/j.1365-2966.2004.07453.xWe analyse the observed correlation between galaxy environment and Hα emission-line strength, using volume-limited samples and group catalogues of 24 968 galaxies at 0.05