VFTS 102 (Czech Wikipedia)

Analysis of information sources in references of the Wikipedia article "VFTS 102" in Czech language version.

refsWebsite

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3doi.org

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3harvard.edu

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99^th place

3arxiv.org

69^th place

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2unistra.fr

low place

1semanticscholar.org

11^th place

313^th place

1roe.ac.uk

low place

arxiv.org (Global: 69^th place; Czech: 196^th place)

DUFTON, P. L. The VLT-FLAMES Tarantula Survey: The Fastest Rotating O-type Star and Shortest Period LMC Pulsar—Remnants of a Supernova Disrupted Binary?. The Astrophysical Journal Letters. 2011, s. L22. doi:10.1088/2041-8205/743/1/L22. Bibcode 2011ApJ...743L..22D. arXiv 1111.0157.
SHEPARD, Katherine. HST/COS Spectra of the Wind Lines of VFTS 102 and 285. The Astrophysical Journal. January 2020, s. 82. doi:10.3847/1538-4357/ab5a82. S2CID 208202016. Bibcode 2020ApJ...888...82S. arXiv 1911.09675.
JIANG, Dengkai; HAN, Zhanwen. The binary merger channel for the progenitor of the fastest rotating O-type star VFTS 102. Monthly Notices of the Royal Astronomical Society. 2013, s. 1218. doi:10.1093/mnras/sts105. Bibcode 2013MNRAS.428.1218J. arXiv 1302.6296.

doi.org (Global: 2^nd place; Czech: 4^th place)

DUFTON, P. L. The VLT-FLAMES Tarantula Survey: The Fastest Rotating O-type Star and Shortest Period LMC Pulsar—Remnants of a Supernova Disrupted Binary?. The Astrophysical Journal Letters. 2011, s. L22. doi:10.1088/2041-8205/743/1/L22. Bibcode 2011ApJ...743L..22D. arXiv 1111.0157.
SHEPARD, Katherine. HST/COS Spectra of the Wind Lines of VFTS 102 and 285. The Astrophysical Journal. January 2020, s. 82. doi:10.3847/1538-4357/ab5a82. S2CID 208202016. Bibcode 2020ApJ...888...82S. arXiv 1911.09675.
JIANG, Dengkai; HAN, Zhanwen. The binary merger channel for the progenitor of the fastest rotating O-type star VFTS 102. Monthly Notices of the Royal Astronomical Society. 2013, s. 1218. doi:10.1093/mnras/sts105. Bibcode 2013MNRAS.428.1218J. arXiv 1302.6296.

harvard.edu (Global: 18^th place; Czech: 99^th place)

adsabs.harvard.edu

DUFTON, P. L. The VLT-FLAMES Tarantula Survey: The Fastest Rotating O-type Star and Shortest Period LMC Pulsar—Remnants of a Supernova Disrupted Binary?. The Astrophysical Journal Letters. 2011, s. L22. doi:10.1088/2041-8205/743/1/L22. Bibcode 2011ApJ...743L..22D. arXiv 1111.0157.
SHEPARD, Katherine. HST/COS Spectra of the Wind Lines of VFTS 102 and 285. The Astrophysical Journal. January 2020, s. 82. doi:10.3847/1538-4357/ab5a82. S2CID 208202016. Bibcode 2020ApJ...888...82S. arXiv 1911.09675.
JIANG, Dengkai; HAN, Zhanwen. The binary merger channel for the progenitor of the fastest rotating O-type star VFTS 102. Monthly Notices of the Royal Astronomical Society. 2013, s. 1218. doi:10.1093/mnras/sts105. Bibcode 2013MNRAS.428.1218J. arXiv 1302.6296.

roe.ac.uk (Global: low place; Czech: low place)

ESO VLT Tarantula Survey [online]. [cit. 2025-01-16]. Dostupné online.

semanticscholar.org (Global: 11^th place; Czech: 313^th place)

api.semanticscholar.org

SHEPARD, Katherine. HST/COS Spectra of the Wind Lines of VFTS 102 and 285. The Astrophysical Journal. January 2020, s. 82. doi:10.3847/1538-4357/ab5a82. S2CID 208202016. Bibcode 2020ApJ...888...82S. arXiv 1911.09675.

unistra.fr (Global: low place; Czech: low place)

simbad.cds.unistra.fr

VFTS 102 [online]. SIMBAD Astronomical Database [cit. 2025-01-16]. Dostupné online.

vizier.cds.unistra.fr

VizieR: VFTS 102 [online]. VizieR Online Data Catalog [cit. 2025-01-16]. Dostupné online.