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Cited by
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This article has been cited by the following publications. This list is generated based on data provided by Crossref.
Calderón, Juan P. Bassino, Lilia P. Cellone, Sergio A. Richtler, Tom Caso, Juan P. and Gómez, Matías 2015. Early-type galaxies in the Antlia Cluster: a deep look into scaling relations. Monthly Notices of the Royal Astronomical Society, Vol. 451, Issue. 1, p. 791.
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Schombert, James M. 2015. THE STRUCTURE OF GALAXIES. III. TWO STRUCTURAL FAMILIES OF ELLIPTICALS. The Astronomical Journal, Vol. 150, Issue. 5, p. 162.
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Cooper, A. P. Gao, L. Guo, Q. Frenk, C. S. Jenkins, A. Springel, V. and White, S. D. M. 2015. Surface photometry of brightest cluster galaxies and intracluster stars in ΛCDM. Monthly Notices of the Royal Astronomical Society, Vol. 451, Issue. 3, p. 2703.
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Schombert, James M. 2016. COLORS OF ELLIPTICALS FROM GALEX TO SPITZER. The Astronomical Journal, Vol. 152, Issue. 6, p. 214.
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Schombert, James M. 2017. On the Dichotomy between Normal and Dwarf Ellipticals. Publications of the Astronomical Society of Australia, Vol. 34, Issue. ,
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Schombert, James M. 2018. Colors of Dwarf Ellipticals from GALEX to WISE. The Astronomical Journal, Vol. 155, Issue. 2, p. 69.
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Ríos-López, Emmanuel Añorve, Christopher Ibarra-Medel, Héctor J López-Cruz, Omar Alvira-Enríquez, Joaquín Iacobuta, Gabriela and Valerdi, Mabel 2021. 2D surface brightness modelling of large 2MASS galaxies – I: photometry and structural parameters. Monthly Notices of the Royal Astronomical Society, Vol. 507, Issue. 4, p. 5952.
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The Structure of Galaxies: II. Fitting Functions and Scaling Relations for Ellipticals
  • Volume 30
  • J. M. Schombert (a1)
  • DOI: https://doi.org/10.1017/pas.2013.010
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The Structure of Galaxies: II. Fitting Functions and Scaling Relations for Ellipticals
  • Volume 30
  • J. M. Schombert (a1)
  • DOI: https://doi.org/10.1017/pas.2013.010
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The Structure of Galaxies: II. Fitting Functions and Scaling Relations for Ellipticals
  • Volume 30
  • J. M. Schombert (a1)
  • DOI: https://doi.org/10.1017/pas.2013.010
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