Astrophysics (Index)About

bolometric luminosity

(LBol, luminosity)
(total luminosity of an object at all wavelengths)

Bolometric luminosity (LBol) is an astronomical body's total power output across all EMR wavelengths. A bolometer is a device that measures incoming EMR at all wavelengths (or at least over a significant wavelength-range), and luminosity is the power output of an astronomical body. The term luminosity generally means bolometric luminosity, i.e., when it is unqualified and when context does not imply otherwise. Bolometric magnitude is a kind of logarithmic measure of the same value (presuming the body's EMR output is isotropic, i.e., emitted equally in all directions).


(EMR,physics,luminosity,measure)
Further reading:
https://en.wikipedia.org/wiki/Luminosity#Measurement
https://en.wikipedia.org/wiki/Bolometric_magnitude
https://dictionary.obspm.fr/index.php?formSearchTextfield=bolometric+luminosity&showAll=1
http://astronomy.swin.edu.au/cosmos/L/Luminosity
https://www.atnf.csiro.au/outreach/education/senior/astrophysics/photometry_luminosity.html

Referenced by pages:
A-type star (A)
B-type star (B)
bolometer
effective temperature (Teff)
F-type star (F)
G-type star (G)
hyperluminous infrared galaxy (HLIRG)
K-type star (K)
luminosity (L)
luminous infrared galaxy (LIRG)
M-type star (M)
monochromatic luminosity
O-type star (O)
O5 spectral type (O5)
Stefan-Boltzmann constant (σ)
ultraluminous infrared galaxy (ULIRG)
Wolf 359
Wolf-Rayet star

Index