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| [JRW2004] XMM-14 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST15:39:04 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1997ApJS..112...49M | 196 | 142 | Optically identified supernova remnants in the nearby spiral galaxies: NGC 5204, NGC 5585, NGC 6946, M81, and M101. | MATONICK D.M. and FESEN R.A. | |||||
| 1999ApJ...517L..27W | 2 | 7 | 54 | Detection of x-ray-emitting hypernova remnants in M101. | WANG Q.D. | ||||
| 1999ApJ...523..121W | 83 | 40 | An ultradeep high-resolution X-ray image of M101: the X-ray source population in a late-type spiral. | WANG Q.D., IMMLER S.A. and PIETSCH W. | |||||
| 2000MNRAS.319...17L | 100 | 37 | Multiwavelength study of the nuclei of a volume-limited sample of galaxies - I. X-ray observations. | LIRA P., LAWRENCE A. and JOHNSON R.A. | |||||
| 2001AJ....121.3001S | 9 | 15 | Reconsidering the identification of M101 hypernova remnant candidates. | SNOWDEN S.L., MUKAI K., PENCE W., et al. | |||||
|
2001ApJ...561..189P |
30 | 74 | Chandra X-ray sources in M101. | PENCE W.D., SNOWDEN S.L., MUKAI K., et al. | |||||
| 2003ApJ...582..184M | 1 | 15 | 55 | Chandra observation of luminous and ultraluminous X-ray binaries in M101. | MUKAI K., PENCE W.D., SNOWDEN S.L., et al. | ||||
| 2004MNRAS.349..404J | 52 | 24 | An XMM-Newton view of M101 - I. The luminous X-ray source population. | JENKINS L.P., ROBERTS T.P., WARWICK R.S., et al. | |||||
| 2012AJ....143...85F | 92 | D | X | 3 | 85 | 10 | Physical structure and nature of supernova remnants in M101. | FRANCHETTI N.A., GRUENDL R.A., CHU Y.-H., et al. | |
|
2012ApJ...756...27L |
15 | D | 1 | 4347 | 64 | Classification of X-ray sources in the XMM-Newton serendipitous source catalog. | LIN D., WEBB N.A. and BARRET D. | ||
|
2015MNRAS.446..943V |
16 | D | 1 | 1179 | 6 | Optical supernova remnants in nearby galaxies and their influence on star formation rates derived from Hα emission. | VUCETIC M.M., ARBUTINA B. and UROSEVIC D. | ||
| 2016PASJ...68S..18Y | 39 | X | 1 | 14 | ~ | Iron emission line from the spiral galaxy M101. | YAMAUCHI S. |