霍姆斯彗星 (Chinese Wikipedia)
Analysis of information sources in references of the Wikipedia article "霍姆斯彗星" in Chinese language version.
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aerith.net
- Seiichi Yoshida. 17P/Holmes. Seiichi Yoshida's Comet Catalog. [2010-02-24].
archive.today
- Editors. "Comet Holmes Stays Bright, Enlarges in the Evening Sky Archive.is的存檔，存档日期2007-10-27", Sky and Telescope, 27 October 2007. Retrieved 29 October 2007.
- Roger W. Sinnott. Comet Holmes Undergoes Huge Outburst. Sky & Telescope. October 24, 2007 [2007-10-25]. （原始内容存档于2007-10-27）.
- Comet 17P/Holmes: report on brightest outburst since 2007
arxiv.org
- Altenhoff, W. J.; Kreysa, E.; Menten, K. M.; Sievers, A.; Thum, C.; Weiss, A. Why did Comet 17P/Holmes burst out? Nucleus splitting or delayed sublimation?. Astronomy and Astrophysics. 2009, 495 (3): 975–978. Bibcode:2009A&A...495..975A. arXiv:0901.2739
. doi:10.1051/0004-6361:200810458.
cloudbait.com
- Primary measurements, Chris L. Peterson Cloudbait Observatory, Colorado 互联网档案馆的存檔，存档日期2011-05-25., The coma size values plotted at the bottom of this page are primary measurements. They were obtained using conventional methods: individual short CCDs images were made in order to avoid saturation, and these were then calibrated with bias, flat, and dark frames and summed to increase the image dynamic range. Each stacked image (for the 5 nights of data) was astrometrically calibrated (using Pinpoint) for scale, and the intensity profile of the coma measured with a standard tool (in this case, the line profile tool in MaximDL). The resulting profiles were exported to Excel, normalized to the same gain, and the width measured against the noise floor. The best reference is the plotted data itself.
- Primary measurements, (see luminosity graph; bottom of page) Cloudbait Observatory, Colorado 互联网档案馆的存檔，存档日期2011-05-25.
doi.org
- Gritsevich, M.; Nissinen, M.; Oksanen, A.; Suomela, J.; Silber, E. A. Evolution of the dust trail of comet 17P/Holmes. Monthly Notices of the Royal Astronomical Society. June 2022, 513 (2): 2201–2214. doi:10.1093/mnras/stac822. hdl:10995/117894 .
- Altenhoff, W. J.; Kreysa, E.; Menten, K. M.; Sievers, A.; Thum, C.; Weiss, A. Why did Comet 17P/Holmes burst out? Nucleus splitting or delayed sublimation?. Astronomy and Astrophysics. 2009, 495 (3): 975–978. Bibcode:2009A&A...495..975A. arXiv:0901.2739 . doi:10.1051/0004-6361:200810458.
fc2.com
jcometobs.web.fc2.com
- Kinoshita, Kazuo. 17P/Holmes past, present and future orbital elements. Comet Orbit. 2019-05-22 [2023-07-19]. （原始内容存档于2011-07-10）.
handle.net
hdl.handle.net
- Gritsevich, M.; Nissinen, M.; Oksanen, A.; Suomela, J.; Silber, E. A. Evolution of the dust trail of comet 17P/Holmes. Monthly Notices of the Royal Astronomical Society. June 2022, 513 (2): 2201–2214. doi:10.1093/mnras/stac822. hdl:10995/117894 .
harvard.edu
ui.adsabs.harvard.edu
- Holmes, Edwin. Discovery of a New Comet in Andromeda. The Observatory. 1892, 15: 441–443. Bibcode:1892Obs....15..441H.
- Meeting of the Royal Astronomical Society, Friday, November 11, 1892. The Observatory. 1892, 15: 417–424. Bibcode:1892Obs....15..417..
- Altenhoff, W. J.; Kreysa, E.; Menten, K. M.; Sievers, A.; Thum, C.; Weiss, A. Why did Comet 17P/Holmes burst out? Nucleus splitting or delayed sublimation?. Astronomy and Astrophysics. 2009, 495 (3): 975–978. Bibcode:2009A&A...495..975A. arXiv:0901.2739 . doi:10.1051/0004-6361:200810458.
adsabs.harvard.edu
- Davidson, J. E. "Comet e, 1889," The Observatory, July 1890, Vol. 13, pp. 247. Retrieved 27 October 2007.
minorplanetcenter.net
- 17P/Holmes Orbit. Minor Planet Center. [2021-06-12].
nasa.gov
ssd.jpl.nasa.gov
- Horizons Batch for 17P/Holmes (90000285) on 2028-Jan-31 (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. [2023-02-11]. (JPL#K212/32 Soln.date: 2023-Jan-30)
- Nasa 3D simulation of orbit for 17P/Holmes (Java Applet)
oaa.gr.jp
- Syuichi Nakano. 17P/Holmes (NK 2100). OAA Computing and Minor Planet Sections. 2011-05-19 [2012-02-18]. （原始内容存档于2015-09-11）.
skyandtelescope.com
- Editors. "Comet Holmes Stays Bright, Enlarges in the Evening Sky Archive.is的存檔，存档日期2007-10-27", Sky and Telescope, 27 October 2007. Retrieved 29 October 2007.
- Roger W. Sinnott. Comet Holmes Undergoes Huge Outburst. Sky & Telescope. October 24, 2007 [2007-10-25]. （原始内容存档于2007-10-27）.
space.com
- Britt, Robert. Incredible Comet Bigger than the Sun. Space.com. 2007-11-15 [2008-04-30].
spaceweather.com
- Skymap: late October 2007, Northeast, after sunset, Spaceweather.com. Retrieved 28 October 2007
ucla.edu
www2.ess.ucla.edu
- Jewitt, David. Comet Holmes Bigger Than The Sun. Institute for Astronomy at the University of Hawaii. 2007-11-09 [2007-11-17].
uni-bonn.de
astro.uni-bonn.de
- Fischer, Daniel. "Incredible comet eruption: from under 17th to 3rd magnitude in hours!," The Cosmic Mirror, #306, 24 October 2007. Retrieved 25 October 2007.
usatoday.com
blogs.usatoday.com
- Gunn, Angela. "Flash News Flash! 互联网档案馆的存檔，存档日期2007-06-25.," USA Today Tech Space, 24 October 2007. Retrieved 25 October 2007.
web.archive.org
- Syuichi Nakano. 17P/Holmes (NK 2100). OAA Computing and Minor Planet Sections. 2011-05-19 [2012-02-18]. （原始内容存档于2015-09-11）.
- Kinoshita, Kazuo. 17P/Holmes past, present and future orbital elements. Comet Orbit. 2019-05-22 [2023-07-19]. （原始内容存档于2011-07-10）.
- Gunn, Angela. "Flash News Flash! 互联网档案馆的存檔，存档日期2007-06-25.," USA Today Tech Space, 24 October 2007. Retrieved 25 October 2007.
- Primary measurements, Chris L. Peterson Cloudbait Observatory, Colorado 互联网档案馆的存檔，存档日期2011-05-25., The coma size values plotted at the bottom of this page are primary measurements. They were obtained using conventional methods: individual short CCDs images were made in order to avoid saturation, and these were then calibrated with bias, flat, and dark frames and summed to increase the image dynamic range. Each stacked image (for the 5 nights of data) was astrometrically calibrated (using Pinpoint) for scale, and the intensity profile of the coma measured with a standard tool (in this case, the line profile tool in MaximDL). The resulting profiles were exported to Excel, normalized to the same gain, and the width measured against the noise floor. The best reference is the plotted data itself.
- Primary measurements, (see luminosity graph; bottom of page) Cloudbait Observatory, Colorado 互联网档案馆的存檔，存档日期2011-05-25.