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| NAME NGC 3341B , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST11:28:34 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2008ApJ...683L.119B | 76 | X | 2 | 6 | 27 | An offset Seyfert 2 nucleus in the minor merger system NGC 3341. | BARTH A.J., BENTZ M.C., GREENE J.E., et al. | ||
|
2011ApJ...737..101L |
15 | D | 1 | 2621 | 118 | Active galactic nucleus pairs from the Sloan Digital Sky Survey. I. The frequency on ∼5-100 kpc scales. | LIU X., SHEN Y., STRAUSS M.A., et al. | ||
| 2012MNRAS.420..878K | 15 | D | 1 | 169 | 114 | The galaxy zoo survey for giant AGN-ionized clouds: past and present black hole accretion events. | KEEL W.C., CHOJNOWSKI S.D., BENNERT V.N., et al. | ||
| 2013MNRAS.435.2335B | 1459 | A | D | S X C | 37 | 14 | 12 | The NGC 3341 minor merger: a panchromatic view of the active galactic nucleus in a dwarf companion. | BIANCHI S., PICONCELLI E., PEREZ-TORRES M.A., et al. |
| 2016ApJ...829...37B | 94 | D | X | 3 | 21 | 24 | Spatially offset active galactic nuclei. I. Selection and spectroscopic properties. | BARROWS R.S., COMERFORD J.M., GREENE J.E., et al. | |
| 2017MNRAS.464L..70Y | 40 | X | 1 | 20 | 9 | NGC 5252: a pair of radio-emitting active galactic nuclei? | YANG X., YANG J., PARAGI Z., et al. | ||
|
2019MNRAS.483.4847K |
16 | D | 2 | 228 | ~ | AGN photoionization of gas in companion galaxies as a probe of AGN radiation in time and direction. | KEEL W.C., BENNERT V.N., PANCOAST A., et al. | ||
|
2020ApJ...900...79H |
16 | D | 1 | 138 | 14 | A Chandra X-ray Survey of optically selected AGN pairs. | HOU M., LI Z. and LIU X. | ||
|
2020MNRAS.498.4790K |
16 | D | 1 | 2220 | 47 | A census of ultraluminous X-ray sources in the local Universe. | KOVLAKAS K., ZEZAS A., ANDREWS J.J., et al. | ||
| 2022ApJ...928...73K | 17 | D | 2 | 52 | 3 | Determining Star Formation Rates of Active Galactic Nucleus Host Galaxies Based on SED Fitting with Submillimeter Data. | KIM C., WOO J.-H., JADHAV Y., et al. |