Question

Description acceptable. This process begins when exceeding a limit proportional to the fourth power of the speed of sound over alpha times big-G to the three-halves. (10[1])Edwin Salpeter’s IMF (-5[1])models the results of this process. (10[1])Recent estimates (10[1])suggest that the rate of this process scales with the 1.4th power of the surface gas density by the empirical Kennicutt–Schmidt law. Exceeding the (10[1])Bonnor–Ebert and Jeans masses will begin this process, (10[2])which produces (10[2])T (10[2])Tauri (10[1])objects (10[1]-5[1])that (10[1])then evolve to follow (10[1])the Hayashi (10[1])track downwards. (10[3]-5[2])This process (10[1])begins when a molecular (10[1])cloud in the ISM (10[4])loses (10[2])hydrostatic equilibrium (10[3])and undergoes (10[2])gravitational collapse (10[2]-5[2])so that fusion occurs. (10[3])For 10 points, (10[1])identify this process that creates the objects found (10[1])on Hertzsprung–Russell (10[1])diagrams, (10[2])such as Alpha Centauri. (10[1])■END■ (10[9]0[1])

ANSWER: star formation [or stellar formation or equivalents mentioning the idea of stars being created; accept star formation rate; prompt on SFR; prompt on gravitational collapse until read by asking “what other process does that lead to?”]
<Other Science>
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PlayerTeamOpponentBuzz PositionValue
Shardul ParthasarathyUIUC BPurdue A2510
Cormac StephensonSouthampton ALSE A28-5
Ezra SantosUChicago AUIUC C3410
Athena Shadden (UG)Texas ANYU B3610
Teigue KellyPenn State APenn A6010
Alex AkridgeIndiana AUIUC A6810
Oscar O'FlanaganImperial ABristol B6810
Kevin YeSFUUW A7010
Leo LawUF AUF B7010
Ethan MaUIUC DUChicago D7110
Matthew Wang (UG)UBC AUW B7110
Shiva TegullaUCF AUF C7210
Rohan ShelkeBerkeley BStanford A7310
Allan LeeStanford LStanford M73-5
Geoffrey WuColumbia AJohns Hopkins A7410
June YinWashU BUChicago C7810
Delia CropperOxford ATeam 18010
Swapnil GargBerkeley ABerkeley C8210
Sam Wang (UG)Pitt B (UG)Ohio State B (DII)8210
Mitchell IndekMichigan BOhio State C (DII)8210
Chris LevesleyWarwick ABristol A82-5
Tom HainesDurham AEdinburgh82-5
Jason Thieu (DII)Michigan State B (UG)Kenyon A (UG)8410
Joseph CollinsImperial BWarwick B8810
Samarth RamUChicago BSIUE A9210
Matt SchiavoneNorthwestern AWashU C9210
Dylan Randall (D2)Ole MissWUSTL A9210
Braden Booth (D2)MissouriTexas B9210
Will HollisterLehigh ARutgers C9310
Henry JamesonLSE BCambridge C9310
Jake Meltzer (DII)CWRU A (UG)Michigan State C (UG)9510
Mitchell Hackett (D2)Central OklahomaNYU A9510
Faiz AhmedBirminghamOxford B9510
ArielPitt AMichigan D9710
Christian SherringtonSouthampton ASouthampton B9710
Sam Macchi (D2)Vassar AOregon State99-5
Aryan PathakUF EFlorida Tech A99-5
Rachel BenthamCambridge BSouthampton B9910
Alessandro d'AttanasioCambridge DDurham B9910
Rahul Rao-PothurajuRowan AHaverford A10310
Alejandro Prieto Mendoza (D2)Texas DTexas C10310
Jackson Hopper (UG)Mississippi StateVassar B10310
Hazel DePreist-SullivanBard AColumbia B10610
Nermeen RahmanIndiana BPurdue D11410
Nicholas NguyenUF DFlorida Tech B11610
Thomas FlexerPenn State BPenn B11710
Jonathan Ho (DII)AlbertaUBC B11710
Michal GerasimiukStanford MStanford L12110
Max KoldaNotre DameWashU D12210
Owen Brown (DII)Kenyon B (DII)Michigan C (UG)12210
Ruchir Kodihalli (UG)CWRU B (UG)CWRU D (DII)12210
Brynn JonesOregon StateVassar A12210
Chloe Wei (D2)McGill EArkansas12210
Aidan BernardoFlorida Tech AUF E12210
Juan LandaetaFlorida State University AUCF B12210
Lovel HearnEdinburghDurham A12210
Kevin FlanaganBristol AWarwick A1220
Cormac BeirneLSE ASouthampton A12210