bolometric magnitude

contains detailed tables of bolometric corrections (note that these second set of tables are consistent with a bolometric magnitude of 4.73 for the Sun and

Resolution B2 on Recommended Zero Points for the Absolute and Apparent Bolometric Magnitude Scales (PDF). Resolutions adopted at the General Assemblies (International

吉秒差距（Gpc）則是描述極為遙遠的星系與眾多類星體。 2015年8月，國際天文學聯合會通過B2決議文，將絕對星等與熱星等（英语：bolometric magnitude）進行標準定義，也包含將秒差距定義為一個精確值，即7005648000000000000♠648000/π天文單位，或大約7016308567758149137♠3

亮星列表 巨大恆星列表 恆星亮度列表 巨大質量恆星列表 The bolometric magnitude of Rigel is −7.92m±0.28m. Taking into account the absolute magnitude of Sun (4.83m) this can be recalculated

恆星類型，B型 恆星計數，恆星勘查 Habets, G. M. H. J.; Heintze, J. R. W. Empirical bolometric corrections for the main-sequence. Astronomy and Astrophysics Supplement