Buzzoni et al.: "Optical tracking of the Gaia spacecraft in L2"
Study of blazar activity in 10 year Fermi-LAT data and implications for TeV neutrino expectations
PDF) Universal bolometric corrections for AGN over 7 luminosity decades (2020) | F. Duras | 99 Citations
Fits to Evolutionary Models
Solved A star cluster contains 200 F5 stars at the main | Chegg.com
The star π And A has a visual magnitude V = 4.33. If | Chegg.com
![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/791f0c10e2270f4bc1397f82cecaf22eb7c82006/12-Table12-1.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
7.7.5 Quality assessment and validation‣ 7.7 Long period variables ‣ Chapter 7 Variability ‣ Part III Gaia data analysis ‣ Gaia Data Release 2 Documentation release 1.2
Astronomy Lecture Number 2
arXiv:2103.03258v1 [astro-ph.SR] 4 Mar 2021
Olivier Guyon's webpage
On the zero point constant of the bolometric correction scale - NASA/ADS
Useful Reference Tables of Stellar Properties
Synthetic magnitudes and bolometric corrections | Download Table
Brane Space: Selected Questions -Answers From All Experts Astronomy Forum (Mass-Luminosity Relation)
Frontiers | Parameterizing the AGN Radius–Luminosity Relation from the Eigenvector 1 Viewpoint
8.3.3 Stellar luminosities and radii‣ 8.3 Processing steps: the Apsis modules ‣ Chapter 8 Astrophysical Parameters ‣ Part III Gaia data analysis ‣ Gaia Data Release 2 Documentation release 1.2
4 Observational inputs for the IRFM
Brane Space: Tackling Intermediate Astronomy Problems (8)
4 Observational inputs for the IRFM
arXiv:2103.03258v1 [astro-ph.SR] 4 Mar 2021
Astron. Astrophys. 346, 819-830 (1999)
