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| LEDA 83860 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:48:07 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1990AJ....100....1F |
793 | 168 | Population studies in groups and clusters of galaxies. III. A catalog of galaxies in five nearby groups. | FERGUSON H.C. and SANDAGE A. | |||||
|
1996A&AS..117..467G |
22339 | 19 | An image database. II. Catalogue between δ=-0deg and δ=70deg. | GARNIER R., PATUREL G., PETIT C., et al. | |||||
| 1999A&A...345..403C | 20 | 12 | Surface brightness profiles of dwarf galaxies in the NGC 5044 group: a critical revision of the luminosity - shape relation as a distance indicator. | CELLONE S.A. | |||||
| 2001A&A...369..736Y | 12 | 5 | Surface-brightness profiles of dwarf galaxies in the NGC 5044 Group: Implications for the luminosity-shape and scalelength-shape relationships as distance indicators. | YOUNG C.K. and CURRIE M.J. | |||||
| 2001A&A...369..742C | 12 | 9 | On the shape of luminosity profiles of dwarf galaxies as a distance indicator: the NGC 5044 Group revisited. | CELLONE S.A. and BUZZONI A. | |||||
|
2003A&A...412...45P |
15 | D | 1 | 956189 | 750 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
| 2005MNRAS.356...41C | 53 | 22 | The low-luminosity galaxy population in the NGC5044 Group. | CELLONE S.A. and BUZZONI A. | |||||
| 2008MNRAS.389..749M | 15 | D | 1 | 148 | 14 | The anatomy of the NGC5044 group - I. Group membership and dynamics. | MENDEL J.T., PROCTOR R.N., FORBES D.A., et al. | ||
| 2012MNRAS.420.3427B | 15 | D | 4 | 180 | 7 | Evolutionary properties of the low-luminosity galaxy population in the NGC 5044 group. | BUZZONI A., CELLONE S.A., SARACCO P., et al. | ||
|
2020MNRAS.494.1784A |
16 | D | 1 | 47437 | 9 | Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 Mpc. | ASMUS D., GREENWELL C.L., GANDHI P., et al. |