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mbsig
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There are 5 letters in MBSIG ( B3G2I1M3S1 )
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The M–sigma (or M–σ) relation is an empirical correlation between the stellar velocity dispersion σ of a galaxy bulge and the mass M of the supermassive black hole at its center. * The M–σ relation was first presented in 1999 during a conference at the Institut d'astrophysique de Paris in France. The proposed form of the relation, which was called the "Faber–Jackson law for black holes", was* * * * * * M * * * 10 * * 8 * * * * M * * ⊙ * * * * * * ≈ * 3.1 * * * ( * * * σ * * 200 * * * * k * m * * * * * * * s * * * * − * 1 * * * * * * ) * * * 4 * * * . * * * {\displaystyle {\frac {M}{10^{8}M_{\odot }}}\approx 3.1\left({\frac {\sigma }{200~{\rm {km}}~{\rm {s}}^{-1}}}\right)^{4}.} * where * * * * * M * * ⊙ * * * * * {\displaystyle M_{\odot }} * is the solar mass. Publication of the relation in a refereed journal, by two groups, took place the following year. * One of many recent studies, based on the growing sample of published black hole masses in nearby galaxies, gives * * * * * * * M * * * 10 * * 8 * * * * M * * ⊙ * * * * * * ≈ * 1.9 * * * ( * * * σ * * 200 * * * * k * m * * * * * * * s * * * * − * 1 * * * * * * ) * * * 5.1 * * * . * * * {\displaystyle {\frac {M}{10^{8}M_{\odot }}}\approx 1.9\left({\frac {\sigma }{200~{\rm {km}}~... |