Probing the physics of star formation (ProPStar)

Context. Electron fraction and cosmic-ray ionization rates in star-forming regions are important quantities in astrochemical modeling and are critical to the degree of coupling between neutrals, ions, and electrons, which regulates the dynamics of the magnetic field. However, these are difficult qua...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2024-06, Vol.686
Hauptverfasser:	Pineda, Jaime E, Sipilä, Olli, Segura-Cox, Dominique M, Valdivia-Mena, Maria Teresa, Neri, Roberto, Kuffmeier, Michael, Ivlev, Alexei V, Offner, Stella S R, Maureira, Maria Jose, Caselli, Paola, Spezzano, Silvia, Cunningham, Nichol, Schmiedeke, Anika, Chen, Mike
Format:	Artikel
Sprache:	eng
Schlagworte:	Cosmic rays Electrons Ionization Magnetohydrodynamic turbulence Star & galaxy formation Star formation
Online-Zugang:	Volltext
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