Stellar initial mass function varies with metallicity and time

Most structural and evolutionary properties of galaxies strongly rely on the stellar initial mass function (IMF), namely the distribution of the stellar mass formed in each episode of star formation 1 – 4 . The IMF shapes the stellar population in all stellar systems, and so has become one of the mo...

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Veröffentlicht in:	Nature (London) 2023-01, Vol.613 (7944), p.460-462
Hauptverfasser:	Li, Jiadong, Liu, Chao, Zhang, Zhi-Yu, Tian, Hao, Fu, Xiaoting, Li, Jiao, Yan, Zhi-Qiang
Format:	Artikel
Sprache:	eng
Schlagworte:	639/33/34 639/33/34/867 Astronomical models Astronomy Bias Cold Dwarf stars Galactic evolution Galaxies Humanities and Social Sciences Initial mass function Low mass stars Metallicity Milky Way multidisciplinary Planet formation Science Science (multidisciplinary) Solar neighborhood Star & galaxy formation Star formation Stars Stars & galaxies Stellar age Stellar mass Stellar populations Stellar systems Trends
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