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CN AC114 89 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST23:00:56 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
1987MNRAS.229..423C | 155 | 466 | A spectroscopic study of three rich galaxy clusters at zeta=0.31. | COUCH W.J. and SHARPLES R.M. | |||||
1994ApJ...430..121C | 81 | 227 | Morphological studies of the galaxy populations in distant "Butcher-Oemler" clusters with HST. I. AC 114 at z = 0.31 and Abell 370 at z = 0.37. | COUCH W.J., ELLIS R.S., SHARPLES R.M., et al. | |||||
1996MNRAS.279....1B | 333 | 165 | The life-cycle of star formation in distant clusters. | BARGER A.J., ARAGON-SALAMANCA A., ELLIS R.S., et al. | |||||
1998ApJ...497..188C | 208 | 282 | Morphological studies of the galaxy populations in distant ``Butcher-Oemler'' clusters with the Hubble Space Telescope. II. AC 103, AC 118, and AC 114 at z = 0.31. | COUCH W.J., BARGER A.J., SMAIL I., et al. | |||||
2000AJ....119.2118G | 72 | 21 | E+A galaxies in the near-infrared: broadband photometry. | GALAZ G. | |||||
2001ApJ...549..820C | 600 | 85 | A low global star formation rate in the rich galaxy cluster AC 114 at z=0.32. | COUCH W.J., BALOGH M.L., BOWER R.G., et al. | |||||
2005MNRAS.359.1421P | 13 | 28 | Spatially resolved spectroscopy of the E+A galaxies in the z= 0.32 cluster AC 114. | PRACY M.B., COUCH W.J., BLAKE C., et al. | |||||
2011ApJ...729...22A | 15 | D | 1 | 589 | 13 | A multi-wavelength study of low-redshift clusters of galaxies. I. Comparison of X-ray and mid-infrared selected active galactic nuclei. | ATLEE D.W., MARTINI P., ASSEF R.J., et al. | ||
2012ApJ...761..114A | 15 | D | 1 | 499 | 6 | A multi-wavelength study of low-redshift clusters of galaxies. II. Environmental impact on galaxy growth. | ATLEE D.W. and MARTINI P. | ||
2014MNRAS.438.1038R | 94 | D | F | 4 | 21 | 14 | Caught in the act: cluster `k+a' galaxies as a link between spirals and S0s. | RODRIGUEZ DEL PINO B., BAMFORD S.P., ARAGON-SALAMANCA A., et al. |