HE 1327-2326 (Japanese Wikipedia)

Analysis of information sources in references of the Wikipedia article "HE 1327-2326" in Japanese language version.

refsWebsite

Global rank Japanese rank

7harvard.edu

18^th place

107^th place

7worldcat.org

5^th place

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6arxiv.org

69^th place

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6doi.org

2^nd place

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1u-strasbg.fr

1,342^nd place

415^th place

1unistra.fr

low place

4,760^th place

1subarutelescope.org

low place

1asj.or.jp

low place

2,831^st place

arxiv.org

Frebel, Anna et al. (2005). “Nucleosynthetic signatures of the first stars”. Nature (Springer Science and Business Media LLC) 434 (7035): 871–873. arXiv:astro-ph/0503021. Bibcode: 2005Natur.434..871F. doi:10.1038/nature03455. ISSN 0028-0836.
Korn, A. J. et al. (2009-05-20). “HE 1327-2326, An Unevolved Star with [Fe/H] < -5.0. III. Does its Atmosphere Reflect its Natal Composition?”. The Astrophysical Journal (American Astronomical Society) 698 (1): 410-416. arXiv:0903.3885. Bibcode: 2009ApJ...698..410K. doi:10.1088/0004-637x/698/1/410. ISSN 0004-637X.
Arentsen, A. et al. (2019). “Binarity among CEMP-no stars: an indication of multiple formation pathways?”. Astronomy & Astrophysics (EDP Sciences) 621: A108. arXiv:1811.01975. Bibcode: 2019A&A...621A.108A. doi:10.1051/0004-6361/201834146. ISSN 0004-6361.
Iwamoto, Nobuyuki; Umeda, Hideyuki; Tominaga, Nozomu; Nomoto, Ken'ichi; Maeda, Keiichi (2005-07-15). “The First Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars”. Science (American Association for the Advancement of Science (AAAS)) 309 (5733): 451-453. arXiv:astro-ph/0505524. Bibcode: 2005Sci...309..451I. doi:10.1126/science.1112997. ISSN 0036-8075.
Frebel, Anna et al. (2008). “HE 1327-2326, an Unevolved Star with [Fe/H]<-5.0. II. New 3D-1D Corrected Abundances from a Very Large Telescope UVES Spectrum”. The Astrophysical Journal (American Astronomical Society) 684 (1): 588-602. arXiv:0805.3341. Bibcode: 2008ApJ...684..588F. doi:10.1086/590327. ISSN 0004-637X.
Frebel, Anna et al. (2006-01-24). “The Oxygen Abundance of HE 1327-2326”. The Astrophysical Journal (American Astronomical Society) 638 (1): L17-L20. arXiv:astro-ph/0512543. Bibcode: 2006ApJ...638L..17F. doi:10.1086/500592. ISSN 0004-637X.

asj.or.jp

小宮悠 (2015). “宇宙黎明期の生きた化石：極超金属欠乏星の遍歴をたどる”. 天文月報 108 (8): 511-520. ISSN 0374-2466.

doi.org

Frebel, Anna et al. (2005). “Nucleosynthetic signatures of the first stars”. Nature (Springer Science and Business Media LLC) 434 (7035): 871–873. arXiv:astro-ph/0503021. Bibcode: 2005Natur.434..871F. doi:10.1038/nature03455. ISSN 0028-0836.
Korn, A. J. et al. (2009-05-20). “HE 1327-2326, An Unevolved Star with [Fe/H] < -5.0. III. Does its Atmosphere Reflect its Natal Composition?”. The Astrophysical Journal (American Astronomical Society) 698 (1): 410-416. arXiv:0903.3885. Bibcode: 2009ApJ...698..410K. doi:10.1088/0004-637x/698/1/410. ISSN 0004-637X.
Arentsen, A. et al. (2019). “Binarity among CEMP-no stars: an indication of multiple formation pathways?”. Astronomy & Astrophysics (EDP Sciences) 621: A108. arXiv:1811.01975. Bibcode: 2019A&A...621A.108A. doi:10.1051/0004-6361/201834146. ISSN 0004-6361.
Iwamoto, Nobuyuki; Umeda, Hideyuki; Tominaga, Nozomu; Nomoto, Ken'ichi; Maeda, Keiichi (2005-07-15). “The First Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars”. Science (American Association for the Advancement of Science (AAAS)) 309 (5733): 451-453. arXiv:astro-ph/0505524. Bibcode: 2005Sci...309..451I. doi:10.1126/science.1112997. ISSN 0036-8075.
Frebel, Anna et al. (2008). “HE 1327-2326, an Unevolved Star with [Fe/H]<-5.0. II. New 3D-1D Corrected Abundances from a Very Large Telescope UVES Spectrum”. The Astrophysical Journal (American Astronomical Society) 684 (1): 588-602. arXiv:0805.3341. Bibcode: 2008ApJ...684..588F. doi:10.1086/590327. ISSN 0004-637X.
Frebel, Anna et al. (2006-01-24). “The Oxygen Abundance of HE 1327-2326”. The Astrophysical Journal (American Astronomical Society) 638 (1): L17-L20. arXiv:astro-ph/0512543. Bibcode: 2006ApJ...638L..17F. doi:10.1086/500592. ISSN 0004-637X.

harvard.edu

ui.adsabs.harvard.edu

Frebel, Anna et al. (2005). “Nucleosynthetic signatures of the first stars”. Nature (Springer Science and Business Media LLC) 434 (7035): 871–873. arXiv:astro-ph/0503021. Bibcode: 2005Natur.434..871F. doi:10.1038/nature03455. ISSN 0028-0836.
Korn, A. J. et al. (2009-05-20). “HE 1327-2326, An Unevolved Star with [Fe/H] < -5.0. III. Does its Atmosphere Reflect its Natal Composition?”. The Astrophysical Journal (American Astronomical Society) 698 (1): 410-416. arXiv:0903.3885. Bibcode: 2009ApJ...698..410K. doi:10.1088/0004-637x/698/1/410. ISSN 0004-637X.
Gaia Collaboration. “Gaia DR3 Part 1. Main source”. VizieR On-line Data Catalog: I/355/gaiadr3. Bibcode: 2022yCat.1355....0G.
Arentsen, A. et al. (2019). “Binarity among CEMP-no stars: an indication of multiple formation pathways?”. Astronomy & Astrophysics (EDP Sciences) 621: A108. arXiv:1811.01975. Bibcode: 2019A&A...621A.108A. doi:10.1051/0004-6361/201834146. ISSN 0004-6361.
Iwamoto, Nobuyuki; Umeda, Hideyuki; Tominaga, Nozomu; Nomoto, Ken'ichi; Maeda, Keiichi (2005-07-15). “The First Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars”. Science (American Association for the Advancement of Science (AAAS)) 309 (5733): 451-453. arXiv:astro-ph/0505524. Bibcode: 2005Sci...309..451I. doi:10.1126/science.1112997. ISSN 0036-8075.
Frebel, Anna et al. (2008). “HE 1327-2326, an Unevolved Star with [Fe/H]<-5.0. II. New 3D-1D Corrected Abundances from a Very Large Telescope UVES Spectrum”. The Astrophysical Journal (American Astronomical Society) 684 (1): 588-602. arXiv:0805.3341. Bibcode: 2008ApJ...684..588F. doi:10.1086/590327. ISSN 0004-637X.
Frebel, Anna et al. (2006-01-24). “The Oxygen Abundance of HE 1327-2326”. The Astrophysical Journal (American Astronomical Society) 638 (1): L17-L20. arXiv:astro-ph/0512543. Bibcode: 2006ApJ...638L..17F. doi:10.1086/500592. ISSN 0004-637X.

subarutelescope.org

“すばる望遠鏡、最も重元素の少ない星を発見～第一世代星の元素合成に迫る～”. すばる望遠鏡. (2005年4月13日) 2021年3月17日閲覧。

u-strasbg.fr

simbad.u-strasbg.fr

"HE 1327-2326". SIMBAD. Centre de données astronomiques de Strasbourg. 2022年7月8日閲覧。

unistra.fr

vizier.cds.unistra.fr

Gaia Collaboration. “Gaia DR3 Part 1. Main source”. VizieR On-line Data Catalog: I/355/gaiadr3. Bibcode: 2022yCat.1355....0G.

worldcat.org

search.worldcat.org

Frebel, Anna et al. (2005). “Nucleosynthetic signatures of the first stars”. Nature (Springer Science and Business Media LLC) 434 (7035): 871–873. arXiv:astro-ph/0503021. Bibcode: 2005Natur.434..871F. doi:10.1038/nature03455. ISSN 0028-0836.
Korn, A. J. et al. (2009-05-20). “HE 1327-2326, An Unevolved Star with [Fe/H] < -5.0. III. Does its Atmosphere Reflect its Natal Composition?”. The Astrophysical Journal (American Astronomical Society) 698 (1): 410-416. arXiv:0903.3885. Bibcode: 2009ApJ...698..410K. doi:10.1088/0004-637x/698/1/410. ISSN 0004-637X.
Arentsen, A. et al. (2019). “Binarity among CEMP-no stars: an indication of multiple formation pathways?”. Astronomy & Astrophysics (EDP Sciences) 621: A108. arXiv:1811.01975. Bibcode: 2019A&A...621A.108A. doi:10.1051/0004-6361/201834146. ISSN 0004-6361.
小宮悠 (2015). “宇宙黎明期の生きた化石：極超金属欠乏星の遍歴をたどる”. 天文月報 108 (8): 511-520. ISSN 0374-2466.
Iwamoto, Nobuyuki; Umeda, Hideyuki; Tominaga, Nozomu; Nomoto, Ken'ichi; Maeda, Keiichi (2005-07-15). “The First Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars”. Science (American Association for the Advancement of Science (AAAS)) 309 (5733): 451-453. arXiv:astro-ph/0505524. Bibcode: 2005Sci...309..451I. doi:10.1126/science.1112997. ISSN 0036-8075.
Frebel, Anna et al. (2008). “HE 1327-2326, an Unevolved Star with [Fe/H]<-5.0. II. New 3D-1D Corrected Abundances from a Very Large Telescope UVES Spectrum”. The Astrophysical Journal (American Astronomical Society) 684 (1): 588-602. arXiv:0805.3341. Bibcode: 2008ApJ...684..588F. doi:10.1086/590327. ISSN 0004-637X.
Frebel, Anna et al. (2006-01-24). “The Oxygen Abundance of HE 1327-2326”. The Astrophysical Journal (American Astronomical Society) 638 (1): L17-L20. arXiv:astro-ph/0512543. Bibcode: 2006ApJ...638L..17F. doi:10.1086/500592. ISSN 0004-637X.