On the Mass Accretion Rates of Herbig Ae/Be Stars. Magnetospheric Accretion or Boundary Layer?
Understanding how young stars gain their masses through disk-to-star accretion is of paramount importance in astrophysics. It affects our knowledge about the early stellar evolution, the disk lifetime and dissipation processes, the way the planets form on the smallest scales, or the connection to ma...
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| Format: | Article |
| Language: | English |
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MDPI AG
2020-05-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/8/2/39 |