SN 386 (Japanese Wikipedia)

Analysis of information sources in references of the Wikipedia article "SN 386" in Japanese language version.

refsWebsite

Global rank Japanese rank

18^th place

107^th place

1,342^nd place

415^th place

69^th place

227^th place

2^nd place

6^th place

670^th place

1,631^st place

arxiv.org

Borkowski, K. J. et al. (2016). “G11.2-0.3: the young remnant of a stripped-envelope supernova”. Astrophysical Journal 819: 160. arXiv:1602.03531. Bibcode: 2016ApJ...819..160B. doi:10.3847/0004-637X/819/2/160.
Kaspi, V. M. et al. (2001-10-10). “Chandra X-Ray Observations of G11.2-0.3: Implications for Pulsar Ages”. The Astrophysical Journal 560: 372. arXiv:astro-ph/0107292. Bibcode: 2001ApJ...560..371K. doi:10.1086/322515.

cam.ac.uk

mrao.cam.ac.uk

Galactic SNRs: Detailed Listings

doi.org

Borkowski, K. J. et al. (2016). “G11.2-0.3: the young remnant of a stripped-envelope supernova”. Astrophysical Journal 819: 160. arXiv:1602.03531. Bibcode: 2016ApJ...819..160B. doi:10.3847/0004-637X/819/2/160.
Kaspi, V. M. et al. (2001-10-10). “Chandra X-Ray Observations of G11.2-0.3: Implications for Pulsar Ages”. The Astrophysical Journal 560: 372. arXiv:astro-ph/0107292. Bibcode: 2001ApJ...560..371K. doi:10.1086/322515.

harvard.edu

ui.adsabs.harvard.edu

Clark, D. H.; Stephenson, F. R. (1976). “Which Historical New Stars were Supernovae?” (PDF). Q. J. R. Astron. Soc. 17: 290. Bibcode: 1976QJRAS..17..290C. "The position of the star AD 386 corresponds very well with that of the SNR G11.2-0.3, and this leads us to make the tentative suggestion that this source is the remnant of the star."
Borkowski, K. J. et al. (2016). “G11.2-0.3: the young remnant of a stripped-envelope supernova”. Astrophysical Journal 819: 160. arXiv:1602.03531. Bibcode: 2016ApJ...819..160B. doi:10.3847/0004-637X/819/2/160.
Kaspi, V. M. et al. (2001-10-10). “Chandra X-Ray Observations of G11.2-0.3: Implications for Pulsar Ages”. The Astrophysical Journal 560: 372. arXiv:astro-ph/0107292. Bibcode: 2001ApJ...560..371K. doi:10.1086/322515.

adsabs.harvard.edu

Clark, D. H.; Stephenson, F. R. (1976). “Which Historical New Stars were Supernovae?” (PDF). Q. J. R. Astron. Soc. 17: 290. Bibcode: 1976QJRAS..17..290C. "The position of the star AD 386 corresponds very well with that of the SNR G11.2-0.3, and this leads us to make the tentative suggestion that this source is the remnant of the star."

u-strasbg.fr

simbad.u-strasbg.fr

"SNR G11.2-0.3". SIMBAD. Centre de données astronomiques de Strasbourg. 2016年5月23日閲覧。
“SIMBAD Astronomical Database”. Results for PSR J1811-1926. 2016年5月23日閲覧。