V354 Cephei (section Distance)
bolometric magnitude. The bolometric magnitude is converted to solar luminosites in the equation (L = 10^(0.4*(4.74-(Mbol)))), where L is the luminosity...
13 KB (1,460 words) - 20:33, 14 September 2024
are stars at the end of the main sequence, with low temperatures, low luminosites and sizes similar to Jupiter. It is spinning at a rotational velocity...
11 KB (998 words) - 13:34, 24 September 2024
Courbe de rotation et luminosité d'astéroïdes, de comètes et d'étoiles variables". obswww.unige.ch. Retrieved 8 January 2024. – Observatoire de Genève...
20 KB (1,343 words) - 08:02, 2 August 2024
wavelength range. At the highest luminosities, the sample galaxies had luminosites approaching those of high-redshift Lyman-break galaxy. In January 2014...
100 KB (12,658 words) - 01:42, 8 November 2024