مستعر أعظم SN 2011fe (Arabic Wikipedia)

Analysis of information sources in references of the Wikipedia article "مستعر أعظم SN 2011fe" in Arabic language version.

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arxiv.org

Shappee، Benjamin؛ Stanek, Kris (يونيو 2011). "A New Cepheid Distance to the Giant Spiral M101 Based on Image Subtraction of Hubble Space Telescope/Advanced Camera for Surveys Observations". Astrophysical Journal. ج. 733 ع. 2: 124. arXiv:1012.3747. Bibcode:2011ApJ...733..124S. DOI:10.1088/0004-637X/733/2/124.
Perlmutter، S.؛ وآخرون (1999). "Measurements of Omega and Lambda from 42 high redshift supernovae". Astrophysical Journal. ج. 517 ع. 2: 565–86. arXiv:astro-ph/9812133. Bibcode:1999ApJ...517..565P. DOI:10.1086/307221.

http://www.astronomerstelegram.org/?read=3597 EVLA Radio Observations of SN 2011fe نسخة محفوظة 2023-02-05 على موقع واي باك مشين.
Weidong Li؛ وآخرون (25 أغسطس 2011). "Further Analysis of the archival HST images of PTF11kly in M101". The Astronomer's Telegram. مؤرشف من الأصل في 2023-02-05. اطلع عليه بتاريخ 2011-08-25.
S. J. Smartt؛ وآخرون (1 سبتمبر 2011). "No progenitor detection for PTF11kly/SN2011fe in Hubble Space Telescope pre-explosion images". The Astronomer's Telegram. مؤرشف من الأصل في 2023-03-31. اطلع عليه بتاريخ 2011-09-06. [The ]detection limit is still not deep enough to place restrictive limits on the binary companion to the white dwarf. Low-mass red giants and main-sequence stars below about 5 solar masses would remain undetected.

Shappee، Benjamin؛ Stanek, Kris (يونيو 2011). "A New Cepheid Distance to the Giant Spiral M101 Based on Image Subtraction of Hubble Space Telescope/Advanced Camera for Surveys Observations". Astrophysical Journal. ج. 733 ع. 2: 124. arXiv:1012.3747. Bibcode:2011ApJ...733..124S. DOI:10.1088/0004-637X/733/2/124.
Perlmutter، S.؛ وآخرون (1999). "Measurements of Omega and Lambda from 42 high redshift supernovae". Astrophysical Journal. ج. 517 ع. 2: 565–86. arXiv:astro-ph/9812133. Bibcode:1999ApJ...517..565P. DOI:10.1086/307221.

Shappee، Benjamin؛ Stanek, Kris (يونيو 2011). "A New Cepheid Distance to the Giant Spiral M101 Based on Image Subtraction of Hubble Space Telescope/Advanced Camera for Surveys Observations". Astrophysical Journal. ج. 733 ع. 2: 124. arXiv:1012.3747. Bibcode:2011ApJ...733..124S. DOI:10.1088/0004-637X/733/2/124.
Perlmutter، S.؛ وآخرون (1999). "Measurements of Omega and Lambda from 42 high redshift supernovae". Astrophysical Journal. ج. 517 ع. 2: 565–86. arXiv:astro-ph/9812133. Bibcode:1999ApJ...517..565P. DOI:10.1086/307221.

Hartmut Frommert؛ Christine Kronberg (15 سبتمبر 2011). "Supernova 2011fe in M101". مؤرشف من الأصل في 2022-12-06. اطلع عليه بتاريخ 2011-09-17.

"Berkeley Scientists Discover an "Instant Cosmic Classic" Supernova". 25 أغسطس 2011. مؤرشف من الأصل في 2023-02-03.
Hartmut Frommert؛ Christine Kronberg (15 سبتمبر 2011). "Supernova 2011fe in M101". مؤرشف من الأصل في 2022-12-06. اطلع عليه بتاريخ 2011-09-17.
"[vsnet-recent-sn 2676] SN2011ht recent (Cont'd)". مؤرشف من الأصل في 2022-12-06.
http://www.astronomerstelegram.org/?read=3597 EVLA Radio Observations of SN 2011fe نسخة محفوظة 2023-02-05 على موقع واي باك مشين.
Weidong Li؛ وآخرون (25 أغسطس 2011). "Further Analysis of the archival HST images of PTF11kly in M101". The Astronomer's Telegram. مؤرشف من الأصل في 2023-02-05. اطلع عليه بتاريخ 2011-08-25.
S. J. Smartt؛ وآخرون (1 سبتمبر 2011). "No progenitor detection for PTF11kly/SN2011fe in Hubble Space Telescope pre-explosion images". The Astronomer's Telegram. مؤرشف من الأصل في 2023-03-31. اطلع عليه بتاريخ 2011-09-06. [The ]detection limit is still not deep enough to place restrictive limits on the binary companion to the white dwarf. Low-mass red giants and main-sequence stars below about 5 solar masses would remain undetected.