bolometric magnitude

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

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

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