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| SNR G123.1+04.6 , the SIMBAD biblio (14 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST07:36:27 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2021ApJ...918L..33R | 1090 | A | D | X C | 26 | 4 | 14 | The remnant and origin of the historical Supernova 1181 AD. | RITTER A., PARKER Q.A., LYKOU F., et al. |
| 2022MNRAS.517.6183P | 43 | X | 1 | 12 | ~ | WHTZ 1: a high excitation Planetary Nebula not a gaseous cocoon from runaway star HD 185806. | PARKER Q.A., LE DU P., RITTER A., et al. | ||
| 2023ApJ...945L...4F | 2377 | T A | S X C | 52 | 13 | 3 |
Discovery of an Exceptional Optical Nebulosity in the Suspected Galactic SN Iax Remnant Pa 30 Linked to the Historical Guest Star of 1181 CE. |
FESEN R.A., SCHAEFER B.E. and PATCHICK D. | |
| 2023MNRAS.523.3885S | 5484 | A | D | S X C F | 124 | 31 | 2 | The path from the Chinese and Japanese observations of supernova 1181 AD, to a Type Iax supernova, to the merger of CO and ONe white dwarfs. | SCHAEFER B.E. |
| 2023MNRAS.524.1031Y | 44 | X | 1 | 5 | ~ | Observational signatures of carbon-oxygen white dwarf merger remnants. | YAO P.Z., QUATAERT E. and GOULDING A. | ||
| 2023MNRAS.526.1112D | 44 | X | 1 | 24 | ~ | Detection of optical emission from the supernova remnant G7.7-3.7. | DOMCEK V., HERNANDEZ SANTISTEBAN J.V., CHIOTELLIS A., et al. | ||
| 2024MNRAS.531.2422T | 582 | X C | 12 | 22 | ~ | Peering into the Wolf-Rayet phenomenon through [WO] and [WC] stars. | TOALA J.A., TODT H. and SANDER A.A.C. | ||
| 2024ApJ...975L...7C | 878 | T A | X | 19 | 5 | ~ |
Expansion Properties of the Young Supernova Type Iax Remnant Pa 30 Revealed. |
CUNNINGHAM T., CAIAZZO I., PRUSINSKI N.Z., et al. | |
| 2025ApJ...986...93G | 121 | A | X | 3 | 3 | ~ | Methods to Test the Source of the Extreme Gas Motions in WS 35. | GUNDERSON S.J., IGNACE R. and GOLAY W.W. | |
| 2025A&A...699A..33B | 47 | X | 1 | 6 | ~ | A polarized view of the young pulsar wind nebula 3C 58 with IXPE. | BUCCIANTINI N., WONG J., ROMANI R.W., et al. | ||
| 2025ApJ...992L...6S | 3079 | T A | D | S X C | 64 | 11 | ~ |
Absence of Radio Emission Reveals an Exceptionally Weak Explosion of the Putative Historical Supernova Pa 30. |
SHAO Y.-X., ZHOU P., ZHANG X., et al. |
| 2026ApJ...996L...3C | 1330 | T A | X C | 25 | 2 | ~ |
A Wind-driven Origin for the Firework Morphology of the Supernova Remnant Pa 30. |
COUGHLIN E.R., SALVESEN G. and PASHAM D.R. | |
| 2026ApJ...998..240S | 50 | X | 1 | 10 | ~ | The Remarkable Late-time Flux Excess in Hubble Space Telescope Observations of the Type Iax Supernova 2012Z. | SCHWAB M., KWOK L.A., JHA S.W., et al. | ||
| 2026ApJ...999..234K | 150 | X | 3 | 18 | ~ | Type Iax Supernovae as a Source of Iron-rich Silicate Dust. | KUMAR A. and SARANGI A. |