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| KPAIR J1406+5043 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST21:49:01 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1994ApJ...430..179Z | 67 | 13 | Interaction, star formation and HI deficiency in E+S pairs. | ZASOV A.V. and SULENTIC J.W. | |||||
1995A&AS..110..131R 
|
17 | 23 | Gaseous and stellar components in mixed pairs of galaxies. I. The data. | RAMPAZZO R., REDUZZI L., SULENTIC J.W., et al. | |||||
|
1998A&A...330..423R
|
31 | 11 | Testing the physical reality of binaries and compact groups. Properties of early-type galaxies in groups with diffuse X-ray emission. | RAMPAZZO R., COVINO S., TRINCHIERI G., et al. | |||||
| 1998ApJ...493...54C | 85 | 84 | A medium survey of the hard X-ray sky with the ASCA gas imaging spectrometer: the (2-10 keV) number counts relationship. | CAGNONI I., DELLA CECA R. and MACCACARO T. | |||||
| 2005AJ....129.2579D | 105 | 18 | Mixed-morphology pairs as a breeding ground for active nuclei. | DOMINGUE D.L., SULENTIC J.W. and DURBALA A. | |||||
|
2016ApJS..222...16C
|
16 | D | 1 | 399 | 17 | Herschel observations of Major merger pairs at z = 0: dust mass and star formation. | CAO C., XU C.K., DOMINGUE D., et al. | ||
|
2016A&A...588A..14T
|
16 | D | 1 | 84079 | 35 | Friends-of-friends galaxy group finder with membership refinement. | TEMPEL E., KIPPER R., TAMM A., et al. | ||
| 2018ApJS..237....2Z | 16 | D | 1 | 77 | 5 | H I observations of major-merger pairs at z = 0: atomic gas and star formation. | ZUO P., XU C.K., YUN M.S., et al. | ||
|
2018A&A...618A..81T
|
16 | D | 1 | 50420 | 14 | Bayesian group finder based on marked point processes. Method and feasibility study using the 2MRS data set. | TEMPEL E., KRUUSE M., KIPPER R., et al. | ||
|
2019A&A...627A.107L
|
16 | D | 1 | 131 | ~ | CO observations of major merger pairs at z = 0: molecular gas mass and star formation. | LISENFELD U., XU C.K., GAO Y., et al. |
