In astronomy, the bolometric correction is the correction made to the absolute magnitude of an object in order to convert its visible magnitude to its bolometric magnitude. It is large for stars which radiate most of their energy outside of the visible range. A uniform scale for the correction has not yet been standardized.
and 20 Related for: Bolometric correction information
the bolometriccorrection is the correction made to the absolute magnitude of an object in order to convert its visible magnitude to its bolometric magnitude...
star observed only in the infrared. Bolometric luminosities can also be calculated using a bolometriccorrection to a luminosity in a particular passband...
absolute magnitude in a specific filter band to absolute bolometric magnitude, a bolometriccorrection (BC) is applied. In stellar and galactic astronomy,...
magnitude −5, with some examples around −2 (e.g. 14 Persei). With bolometriccorrections around zero, they may only be a few hundred times the luminosity...
99% of the radiation to be emitted outside the visual range (a bolometriccorrection around −5). R136a1 is over forty times the radius of the Sun (42...
the bolometric magnitude 4.54 ± 0.06 and the bolometriccorrection −0.12 ± 0.05 using the formula: BC = Mbol − MV Calculated from the bolometric magnitude...
that humans are able to see), something known as the bolometriccorrection, this star has a bolometric luminosity 1.2% of the Sun's total luminosity. A planet...
each star, and a correction for interstellar extinction. The entries in the list below are further corrected to provide the bolometric magnitude, i.e....
{\displaystyle B-V=M_{B}-M_{V}\!\,} dimensionless dimensionless Bolometriccorrection Cbol (No standard symbol) C b o l = m b o l − V = M b o l − M V...
luminosity and apply a bolometriccorrection to give the total luminosity at all wavelengths, although the size of the bolometriccorrection is extremely sensitive...
estimate K corrections to these measurements in order to make comparisons. If one could measure all wavelengths of light from an object (a bolometric flux)...
respectively). The zero point of the apparent bolometric magnitude scale is based on the definition that an apparent bolometric magnitude of 0 mag is equivalent to...
supernova candidates Lyman, J. D.; Bersier, D.; James, P. A. (2013). "Bolometriccorrections for optical light curves of core-collapse supernovae". Monthly Notices...
by B.W Caroll and D.A Ostlie 1996 edition, chapter 8 Empirical bolometriccorrections for the main-sequence Archived 9 November 2017 at the Wayback Machine...
175B. Habets, G. M. H. J.; Heintz, J. R. W. (1981). "Empirical bolometriccorrections for the main-sequence". Astronomy and Astrophysics Supplement Series...
Eric E. (1 September 2013). "Intrinsic Colors, Temperatures, and BolometricCorrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement...
Castelli, F.; Plez, B. (1998). "Model atmospheres broad-band colors, bolometriccorrections and temperature calibrations for O–M stars". Astronomy and Astrophysics...