GW Orionis (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "GW Orionis" in English language version.

refsWebsite

Global rank English rank

10harvard.edu

18^th place

17^th place

9doi.org

2^nd place

7arxiv.org

69^th place

59^th place

6semanticscholar.org

11^th place

8^th place

3aanda.org

5,591^st place

5,552^nd place

2u-strasbg.fr

1,342^nd place

1,819^th place

aanda.org

Fang, M.; et al. (2014). "GW Orionis: Inner disk readjustments in a triple system". Astronomy and Astrophysics. 570. A118. arXiv:1407.4959. Bibcode:2014A&A...570A.118F. doi:10.1051/0004-6361/201424146. S2CID 119210837.
Berger, J.-P.; et al. (2011). "First astronomical unit scale image of the GW Orionis triple system". Astronomy and Astrophysics Letters. 529. L1. arXiv:1103.3888. Bibcode:2011A&A...529L...1B. doi:10.1051/0004-6361/201016219. S2CID 14305837.
Fang, M.; et al. (2017). "Millimeter observations of the disk around GW Orionis". Astronomy and Astrophysics. 603. A132. arXiv:1705.01917. Bibcode:2017A&A...603A.132F. doi:10.1051/0004-6361/201628792. S2CID 119328687.

arxiv.org

Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
Fang, M.; et al. (2014). "GW Orionis: Inner disk readjustments in a triple system". Astronomy and Astrophysics. 570. A118. arXiv:1407.4959. Bibcode:2014A&A...570A.118F. doi:10.1051/0004-6361/201424146. S2CID 119210837.
Prato, L.; et al. (2018). "Orbital Solution for the Spectroscopic Binary in the GW Ori Hierarchical Triple". The Astrophysical Journal. 852 (1). 38. arXiv:1711.09449. Bibcode:2018ApJ...852...38P. doi:10.3847/1538-4357/aa98df. S2CID 119238386.
Czekala, Ian; et al. (2017). "The Architecture of the GW Ori Young Triple-star System and Its Disk: Dynamical Masses, Mutual Inclinations, and Recurrent Eclipses". The Astrophysical Journal. 851 (2). 132. arXiv:1710.03153. Bibcode:2017ApJ...851..132C. doi:10.3847/1538-4357/aa9be7. S2CID 73629935. When we combined the RV constraints with the disk-based constraint on M_tot, we found stellar masses of M_A = 2.7 M_⊙, M_B = 1.7 M_⊙, and M_C = 0.9 M_⊙, to a precision of ± 0.3 M_⊙
Bi, Jiaqing; et al. (2020). "GW Ori: Interactions between a Triple-star System and Its Circumtriple Disk in Action". The Astrophysical Journal. 895 (1). L18. arXiv:2004.03135. Bibcode:2020ApJ...895L..18B. doi:10.3847/2041-8213/ab8eb4. The stellar masses have been constrained to be ~2.7, 1.7, and 0.9 M_⊙, respectively (Czekala et al. 2017)
Berger, J.-P.; et al. (2011). "First astronomical unit scale image of the GW Orionis triple system". Astronomy and Astrophysics Letters. 529. L1. arXiv:1103.3888. Bibcode:2011A&A...529L...1B. doi:10.1051/0004-6361/201016219. S2CID 14305837.
Fang, M.; et al. (2017). "Millimeter observations of the disk around GW Orionis". Astronomy and Astrophysics. 603. A132. arXiv:1705.01917. Bibcode:2017A&A...603A.132F. doi:10.1051/0004-6361/201628792. S2CID 119328687.

doi.org

Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
Fang, M.; et al. (2014). "GW Orionis: Inner disk readjustments in a triple system". Astronomy and Astrophysics. 570. A118. arXiv:1407.4959. Bibcode:2014A&A...570A.118F. doi:10.1051/0004-6361/201424146. S2CID 119210837.
Prato, L.; et al. (2018). "Orbital Solution for the Spectroscopic Binary in the GW Ori Hierarchical Triple". The Astrophysical Journal. 852 (1). 38. arXiv:1711.09449. Bibcode:2018ApJ...852...38P. doi:10.3847/1538-4357/aa98df. S2CID 119238386.
Czekala, Ian; et al. (2017). "The Architecture of the GW Ori Young Triple-star System and Its Disk: Dynamical Masses, Mutual Inclinations, and Recurrent Eclipses". The Astrophysical Journal. 851 (2). 132. arXiv:1710.03153. Bibcode:2017ApJ...851..132C. doi:10.3847/1538-4357/aa9be7. S2CID 73629935. When we combined the RV constraints with the disk-based constraint on M_tot, we found stellar masses of M_A = 2.7 M_⊙, M_B = 1.7 M_⊙, and M_C = 0.9 M_⊙, to a precision of ± 0.3 M_⊙
Bi, Jiaqing; et al. (2020). "GW Ori: Interactions between a Triple-star System and Its Circumtriple Disk in Action". The Astrophysical Journal. 895 (1). L18. arXiv:2004.03135. Bibcode:2020ApJ...895L..18B. doi:10.3847/2041-8213/ab8eb4. The stellar masses have been constrained to be ~2.7, 1.7, and 0.9 M_⊙, respectively (Czekala et al. 2017)
Mathieu, Robert D.; et al. (1991). "The T Tauri spectroscopic binary GW Orionis". The Astronomical Journal. 101: 2184–2198. Bibcode:1991AJ....101.2184M. doi:10.1086/115841.
Joy, Alfred H.; Wilson, Ralph E. (1949). "Stars whose Spectra have Bright H and K Lines of Calcium". The Astrophysical Journal. 109: 231–243. Bibcode:1949ApJ...109..231J. doi:10.1086/145126.
Berger, J.-P.; et al. (2011). "First astronomical unit scale image of the GW Orionis triple system". Astronomy and Astrophysics Letters. 529. L1. arXiv:1103.3888. Bibcode:2011A&A...529L...1B. doi:10.1051/0004-6361/201016219. S2CID 14305837.
Fang, M.; et al. (2017). "Millimeter observations of the disk around GW Orionis". Astronomy and Astrophysics. 603. A132. arXiv:1705.01917. Bibcode:2017A&A...603A.132F. doi:10.1051/0004-6361/201628792. S2CID 119328687.

harvard.edu

ui.adsabs.harvard.edu

Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
Shevchenko, V. S.; et al. (1998). "The quasi-Algol GW Ori: The nature of eclipses and estimation of the component masses". Astronomy Letters. 24 (4): 528–534. Bibcode:1998AstL...24..528S.
Fang, M.; et al. (2014). "GW Orionis: Inner disk readjustments in a triple system". Astronomy and Astrophysics. 570. A118. arXiv:1407.4959. Bibcode:2014A&A...570A.118F. doi:10.1051/0004-6361/201424146. S2CID 119210837.
Prato, L.; et al. (2018). "Orbital Solution for the Spectroscopic Binary in the GW Ori Hierarchical Triple". The Astrophysical Journal. 852 (1). 38. arXiv:1711.09449. Bibcode:2018ApJ...852...38P. doi:10.3847/1538-4357/aa98df. S2CID 119238386.
Czekala, Ian; et al. (2017). "The Architecture of the GW Ori Young Triple-star System and Its Disk: Dynamical Masses, Mutual Inclinations, and Recurrent Eclipses". The Astrophysical Journal. 851 (2). 132. arXiv:1710.03153. Bibcode:2017ApJ...851..132C. doi:10.3847/1538-4357/aa9be7. S2CID 73629935. When we combined the RV constraints with the disk-based constraint on M_tot, we found stellar masses of M_A = 2.7 M_⊙, M_B = 1.7 M_⊙, and M_C = 0.9 M_⊙, to a precision of ± 0.3 M_⊙
Bi, Jiaqing; et al. (2020). "GW Ori: Interactions between a Triple-star System and Its Circumtriple Disk in Action". The Astrophysical Journal. 895 (1). L18. arXiv:2004.03135. Bibcode:2020ApJ...895L..18B. doi:10.3847/2041-8213/ab8eb4. The stellar masses have been constrained to be ~2.7, 1.7, and 0.9 M_⊙, respectively (Czekala et al. 2017)
Mathieu, Robert D.; et al. (1991). "The T Tauri spectroscopic binary GW Orionis". The Astronomical Journal. 101: 2184–2198. Bibcode:1991AJ....101.2184M. doi:10.1086/115841.
Joy, Alfred H.; Wilson, Ralph E. (1949). "Stars whose Spectra have Bright H and K Lines of Calcium". The Astrophysical Journal. 109: 231–243. Bibcode:1949ApJ...109..231J. doi:10.1086/145126.
Berger, J.-P.; et al. (2011). "First astronomical unit scale image of the GW Orionis triple system". Astronomy and Astrophysics Letters. 529. L1. arXiv:1103.3888. Bibcode:2011A&A...529L...1B. doi:10.1051/0004-6361/201016219. S2CID 14305837.
Fang, M.; et al. (2017). "Millimeter observations of the disk around GW Orionis". Astronomy and Astrophysics. 603. A132. arXiv:1705.01917. Bibcode:2017A&A...603A.132F. doi:10.1051/0004-6361/201628792. S2CID 119328687.

semanticscholar.org

api.semanticscholar.org

Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
Fang, M.; et al. (2014). "GW Orionis: Inner disk readjustments in a triple system". Astronomy and Astrophysics. 570. A118. arXiv:1407.4959. Bibcode:2014A&A...570A.118F. doi:10.1051/0004-6361/201424146. S2CID 119210837.
Prato, L.; et al. (2018). "Orbital Solution for the Spectroscopic Binary in the GW Ori Hierarchical Triple". The Astrophysical Journal. 852 (1). 38. arXiv:1711.09449. Bibcode:2018ApJ...852...38P. doi:10.3847/1538-4357/aa98df. S2CID 119238386.
Czekala, Ian; et al. (2017). "The Architecture of the GW Ori Young Triple-star System and Its Disk: Dynamical Masses, Mutual Inclinations, and Recurrent Eclipses". The Astrophysical Journal. 851 (2). 132. arXiv:1710.03153. Bibcode:2017ApJ...851..132C. doi:10.3847/1538-4357/aa9be7. S2CID 73629935. When we combined the RV constraints with the disk-based constraint on M_tot, we found stellar masses of M_A = 2.7 M_⊙, M_B = 1.7 M_⊙, and M_C = 0.9 M_⊙, to a precision of ± 0.3 M_⊙
Berger, J.-P.; et al. (2011). "First astronomical unit scale image of the GW Orionis triple system". Astronomy and Astrophysics Letters. 529. L1. arXiv:1103.3888. Bibcode:2011A&A...529L...1B. doi:10.1051/0004-6361/201016219. S2CID 14305837.
Fang, M.; et al. (2017). "Millimeter observations of the disk around GW Orionis". Astronomy and Astrophysics. 603. A132. arXiv:1705.01917. Bibcode:2017A&A...603A.132F. doi:10.1051/0004-6361/201628792. S2CID 119328687.

u-strasbg.fr

vizier.u-strasbg.fr

Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.

simbad.u-strasbg.fr

"GW Ori". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-03-21.