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Bolometric correction

  • Luminosity - Wikipedia

    Luminosity - Wikipedia

  • Diameter and Photospheric Structures of Canopus from AMBER/VLTI Interferometry�,

    Diameter and Photospheric Structures of Canopus from AMBER/VLTI Interferometry,

  • On the Zero Point Constant of the Bolometric Correction Scale

    On the Zero Point Constant of the Bolometric Correction Scale

  • Photometry Rule of Thumb

    Photometry Rule of Thumb

  • Astronomy and Astrophysics

    Astronomy and Astrophysics

  • Model Atmospheres Broad-Band Colors, Bolometric Corrections and Temperature Calibrations Foro-Mstars?

    Model Atmospheres Broad-Band Colors, Bolometric Corrections and Temperature Calibrations Foro-Mstars?

  • Measuring the Properties of Stars and Galaxies

    Measuring the Properties of Stars and Galaxies

  • Bolometric Correction for Brown Dwarfs

    Bolometric Correction for Brown Dwarfs

  • Universal Bolometric Corrections for Active Galactic Nuclei Over Seven Luminosity Decades F

    Universal Bolometric Corrections for Active Galactic Nuclei Over Seven Luminosity Decades F

  • Notes on Stars

    Notes on Stars

  • Fundamental Parameters and Spectral Energy Distributions Of

    Fundamental Parameters and Spectral Energy Distributions Of

  • Canopus Angular Diameter Revisited by the AMBER Instrument of the VLT Interferometer

    Canopus Angular Diameter Revisited by the AMBER Instrument of the VLT Interferometer

  • Chapter 7: from Theory to Observations

    Chapter 7: from Theory to Observations

  • Photometry Stellar Photometry: Implementation

    Photometry Stellar Photometry: Implementation

  • YBC: a Stellar Bolometric Corrections Database with Variable Extinction Coefficients

    YBC: a Stellar Bolometric Corrections Database with Variable Extinction Coefficients

  • Stars, Galaxies, and Beyond, 2012

    Stars, Galaxies, and Beyond, 2012

  • Confirmation of the Gaia DR2 Parallax Zero-Point Offset Using

    Confirmation of the Gaia DR2 Parallax Zero-Point Offset Using

  • The R136 Star Cluster Hosts Several Stars Whose Individual Masses Greatly Exceed the Accepted 150 M⊙ Stellar Mass Limit

    The R136 Star Cluster Hosts Several Stars Whose Individual Masses Greatly Exceed the Accepted 150 M⊙ Stellar Mass Limit

Top View
  • A Closer Look at the Alpha Persei Coronal Conundrum
  • On the Use of Empirical Bolometric Corrections for Stars
  • Stellar Temperature Scale and Bolometric Corrections
  • Download This Article in PDF Format
  • Bolometric Correction and Bolometric Magnitude
  • Astronomical Distance Determination
  • YBC, a Stellar Bolometric Corrections Database with Variable Extinction
  • AY 12 Homework #2 Solutions Winter 2016
  • Chap 14 Stellar Spectra and the HR Diagram
  • Synthetic Stellar Photometry – I
  • Bolometric Correction
  • Stage 1: Estimate the Host Star's Absolute Luminosity Based on The
  • The Bolometric Output and Host-Galaxy Properties of Obscured AGN in the XMM-COSMOS Survey
  • The Bolometric Quasar Luminosity Function at Z = 0–7
  • Astronomical Distance Determination
  • Astronomy 142 Recitation #2
  • Acoustic Waves, 87–91 Adams–Williamson Equation, 107–111
  • The Magnitude of the Sun, the Stellar Temperature Scale, and Bolometric Corrections


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