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| PN We 2-245 , the SIMBAD biblio (13 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST07:33:27 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1977A&AS...30..335W | 332 | 27 | A list of possible, probable and true planetary nebulae detected since 1966. | WEINBERGER R. | |||||
| 1978IAUS...76...47K | 267 | 45 | New and misclassified planetary nebulae. | KOHOUTEK L. | |||||
| 1981A&AS...43...75M | 39 | 10 | Radio observations of planetary nebulae at 6 cm. | MROSS R., WEINBERGER R. and HARTL H. | |||||
| 1983A&AS...54..315A | 1435 | 15 | Index and cross-identification of planetary nebulae. | ACKER A., MARCOUT J., OCHSENBEIN F., et al. | |||||
| 1992A&AS...95..337T | 925 | 103 | The extinction constants for galactic planetary nebulae. | TYLENDA R., ACKER A., STENHOLM B., et al. | |||||
|
1992ESOPN...1....1A |
1828 | ~ | Strasbourg-ESO Catalogue of Galactic Planetary Nebulae | ACKER A., OCHSENBEIN F., STENHOLM B., et al. | |||||
|
1997ApJS..112..487S |
455 | 190 | Properties that cannot be explained by the progenitors of planetary nebulae. | SOKER N. | |||||
|
1998ApJS..117..361C |
887 | 101 | Planetary nebulae in the NRAO VLA sky survey. | CONDON J.J. and KAPLAN D.L. | |||||
|
2001A&A...378..843K |
14 | D | 2201 | 103 | Version 2000 of the Catalogue of Galactic Planetary Nebulae. | KOHOUTEK L. | |||
|
2002AN....323..484K |
14 | D | 740 | 5 | Accurate coordinates of planetary nebulae. | KOHOUTEK L. and KUHL D. | |||
|
2003A&A...408.1029K |
1323 | 48 | Galactic Planetary Nebulae and their central stars. I. An accurate and homogeneous set of coordinates. | KERBER F., MIGNANI R.P., GUGLIELMETTI F., et al. | |||||
|
2008PASP..120..380W |
15 | D | 467 | 6 | The spatial orientation of planetary nebulae within the Milky way. | WEIDMANN W.A. and DIAZ R.J. | |||
|
2021ApJ...919..121H |
17 | D | 1 | 136 | 3 | Evidence for cold plasma in planetary nebulae from radio observations with the LOw Frequency ARray (LOFAR). | HAJDUK M., HAVERKORN M., SHIMWELL T., et al. |