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2MASX J15074780+0117318 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.7 - 2021.03.01CET16:59:45 |
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 |
---|---|---|---|---|---|---|---|---|---|
2017ApJ...843...16K ![]() |
17 | D | 1 | 12390 | 21 | Galaxy groups within 3500 km s–1. | KOURKCHI E. and TULLY R.B. | ||
2016MNRAS.459.2212M | 100 | D | F | 5 | 141 | 4 | Galaxy evolution in nearby galaxy groups - III. A GALEX view of NGC 5846, the largest group in the local universe. | MARINO A., MAZZEI P., RAMPAZZO R., et al. | |
2015ApJS..217...27A ![]() |
16 | D | 1 | 5847 | 11 | A catalog of visually classified galaxies in the local (z ∼ 0.01) universe. | ANN H.B., SEO M. and HA D.K. | ||
2010A&A...511A..12E ![]() |
16 | D | 1 | 82 | 9 | Revisiting the low-luminosity galaxy population of the NGC 5846 group with SDSS. | EIGENTHALER P. and ZEILINGER W.W. | ||
2007MNRAS.379.1227H | 92 | D | F | 5 | 31 | 12 | The HI content of elliptical and lenticular galaxies with recent star formation. | HELMBOLDT J.F. | |
2005AJ....130.1502M ![]() |
15 | D | 327 | 52 | The NGC 5846 group: dynamics and the luminosity function to mR=-12. | MAHDAVI A., TRENTHAM N. and TULLY R.B. | |||
2003A&A...412...45P ![]() |
15 | D | 1 | 956233 | 675 | HYPERLEDA. I. Identification and designation of galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
2003AJ....126.1707G ![]() |
421 | 7 | Companions of bright barred Shapley-Ames galaxies. | GARCIA-BARRETO J.A., CARRILLO R. and VERA-VILLAMIZAR N. | |||||
2001MNRAS.325..693H | 210 | 52 | X-ray luminosities of galaxies in groups. | HELSDON S.F., PONMAN T.J., O'SULLIVAN E., et al. | |||||
1999A&AS..140...89P ![]() |
15 | D | 1 | 16700 | 9 | Galaxy coordinates. II. Accurate equatorial coordinates for 17298 galaxies. | PATUREL G., PETIT C., PRUGNIEL P., et al. | ||
1998ApJ...496...39Z ![]() |
1015 | 337 | The properties of poor groups of galaxies. I. Spectroscopic survey and results. | ZABLUDOFF A.I. and MULCHAEY J.S. |
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