Question

An ALMA large program is currently studying how anomalously top-heavy distributions of this quantity may arise from a related distribution for cores. Codes like MESA express the equation of hydrostatic equilibrium in terms of this Lagrangian coordinate. For a polytrope, this quantity is proportional to the “3 minus n over 1 minus n” power of radius. This quantity’s PDF was approximated as a power law with an exponent of minus 2.35 by Edwin Salpeter; that distribution is this quantity’s (15[1])(*) “initial function.” (10[1])A main sequence star’s luminosity is roughly proportional to the seven-halves power of this quantity. (10[1])A star’s initial value of this quantity determines whether it will become a white dwarf, neutron star, or black hole. For 10 points, Type 1a supernovae occur when a white dwarf’s value of what quantity exceeds the Chandrasekhar limit? ■END■

ANSWER: mass [accept core mass function; accept initial mass function; accept mass coordinate; accept Chandrasekhar mass; prompt on CMF or IMF or ALMA-IMF]
<Science - Other Science - Astronomy>
= Average correct buzz position

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Buzzes

PlayerTeamOpponentBuzz PositionValue
Sam MooreSimple VibesGrzegorz Brzęczyszczykiewicz7815
Joseph KrolCien Años de QuizboledadCambridge8010
Oscar O'FlanaganLimp FranceskitDefying Suavity9510

Summary

2024 ARGOS @ Stanford02/22/2025Y3100%33%0%90.33
2024 ARGOS Online03/22/2025Y3100%33%33%116.00
2024 ARGOS @ Brandeis03/22/2025Y3100%0%0%127.00
2024 ARGOS @ McMaster11/17/2024Y580%0%60%120.75
2024 ARGOS @ Columbia11/23/2024Y3100%0%0%111.00
2024 ARGOS @ Chicago11/23/2024Y6100%17%0%86.67
2024 ARGOS @ Christ's College12/14/2024Y3100%33%0%84.33