Thermodynamic Properties of Carbides, Nitrides, and Other Selected Substances - Page 143 - UNT Digital Library
Astron. Astrophys. 346, 819-830 (1999)
Frontiers | Parameterizing the AGN Radius–Luminosity Relation from the Eigenvector 1 Viewpoint
Solved A star cluster contains 200 F5 stars at the main | Chegg.com
![PDF] Bolometric corrections for optical light curves of core-collapse supernovae | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/361bb6833291befafd558601547f08aca4b6de0d/4-Table1-1.png "PDF] Bolometric corrections for optical light curves of core-collapse supernovae | Semantic Scholar")
PDF] Bolometric corrections for optical light curves of core-collapse supernovae | Semantic Scholar
![PDF] Bolometric correction and spectral energy distribution of cool stars in Galactic clusters | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/791f0c10e2270f4bc1397f82cecaf22eb7c82006/4-Table2-1.png "PDF] Bolometric correction and spectral energy distribution of cool stars in Galactic clusters | Semantic Scholar")
PDF] Bolometric correction and spectral energy distribution of cool stars in Galactic clusters | Semantic Scholar
![PDF] Bolometric correction and spectral energy distribution of cool stars in Galactic clusters | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/791f0c10e2270f4bc1397f82cecaf22eb7c82006/5-Table3-1.png "PDF] Bolometric correction and spectral energy distribution of cool stars in Galactic clusters | Semantic Scholar")
PDF] Bolometric correction and spectral energy distribution of cool stars in Galactic clusters | Semantic Scholar
4 Observational inputs for the IRFM
PDF) Universal bolometric corrections for AGN over 7 luminosity decades (2020) | F. Duras | 99 Citations
Buzzoni et al.: "Bolometric correction of cool stars"
Astronomy Lecture Number 2
Olivier Guyon's webpage
Distance and bolometric correction. | Download Table
Fits to Evolutionary Models
Bolometric magnitudes
Study of blazar activity in 10 year Fermi-LAT data and implications for TeV neutrino expectations
On the zero point constant of the bolometric correction scale - NASA/ADS
arXiv:2103.03258v1 [astro-ph.SR] 4 Mar 2021
Distance and bolometric correction. | Download Table
Brane Space: Tackling Intermediate Astronomy Problems (8)
Distance and bolometric correction. | Download Table
The star π And A has a visual magnitude V = 4.33. If | Chegg.com
