Эпсилон Малого Пса (Russian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Эпсилон Малого Пса" in Russian language version.

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arxiv.org

  • Jönsson H., Holtzman J. A., Allende Prieto C., Cunha K., García-Hernández D. A., Hasselquist S., Masseron T., Osorio Y., Shetrone M., Smith V. et al. APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2020. — Vol. 160, Iss. 3. — ISSN 0004-6256; 1538-3881doi:10.3847/1538-3881/ABA592arXiv:2007.05537
  • Liu Y. J., Tan K. F., Wang L., Zhao G., Sato B., Takeda Y., Li H. N. The lithium abundances of a large sample of red giants (англ.) // The Astrophysical Journal / E. VishniacIOP Publishing, 2014. — Vol. 785, Iss. 2. — P. 94. — ISSN 0004-637X; 1538-4357doi:10.1088/0004-637X/785/2/94arXiv:1404.1687
  • Eggleton, P. P.; Tokovinin, A. A. (September 2008), A catalogue of multiplicity among bright stellar systems, Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  • Reffert, Sabine; et al. (2015), Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity, Astronomy and Astrophysics, 574A (2): 116–129, arXiv:1412.4634, Bibcode:2015A&A...574A.116R, doi:10.1051/0004-6361/201322360, hdl:10722/215277, S2CID 59334290. Values are based on 99% probability it is on the horizontal branch.

doi.org

dx.doi.org

doi.org

  • Eggleton, P. P.; Tokovinin, A. A. (September 2008), A catalogue of multiplicity among bright stellar systems, Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  • Reffert, Sabine; et al. (2015), Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity, Astronomy and Astrophysics, 574A (2): 116–129, arXiv:1412.4634, Bibcode:2015A&A...574A.116R, doi:10.1051/0004-6361/201322360, hdl:10722/215277, S2CID 59334290. Values are based on 99% probability it is on the horizontal branch.
  • Williams, P. M. (February 1975), Stellar compositions from narrow-band photometry - V. Barium abundances for 200 evolved stars, Monthly Notices of the Royal Astronomical Society, 170 (2): 343–362, Bibcode:1975MNRAS.170..343W, doi:10.1093/mnras/170.2.343.

handle.net

hdl.handle.net

harvard.edu

ui.adsabs.harvard.edu

  • Eggleton, P. P.; Tokovinin, A. A. (September 2008), A catalogue of multiplicity among bright stellar systems, Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  • Reffert, Sabine; et al. (2015), Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity, Astronomy and Astrophysics, 574A (2): 116–129, arXiv:1412.4634, Bibcode:2015A&A...574A.116R, doi:10.1051/0004-6361/201322360, hdl:10722/215277, S2CID 59334290. Values are based on 99% probability it is on the horizontal branch.
  • Williams, P. M. (February 1975), Stellar compositions from narrow-band photometry - V. Barium abundances for 200 evolved stars, Monthly Notices of the Royal Astronomical Society, 170 (2): 343–362, Bibcode:1975MNRAS.170..343W, doi:10.1093/mnras/170.2.343.

iop.org

iopscience.iop.org

semanticscholar.org

api.semanticscholar.org

  • Eggleton, P. P.; Tokovinin, A. A. (September 2008), A catalogue of multiplicity among bright stellar systems, Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  • Reffert, Sabine; et al. (2015), Precise radial velocities of giant stars. VII. Occurrence rate of giant extrasolar planets as a function of mass and metallicity, Astronomy and Astrophysics, 574A (2): 116–129, arXiv:1412.4634, Bibcode:2015A&A...574A.116R, doi:10.1051/0004-6361/201322360, hdl:10722/215277, S2CID 59334290. Values are based on 99% probability it is on the horizontal branch.

wikidata.org

wikipedia.org

en.wikipedia.org

worldcat.org