柯理思 Flores Gonzalez, Christian Alejandro
Postdoc Fellow
辦公室: ASMAB 1220
電子信箱:
cafloresasiaa.sinica.edu.tw
研究興趣
I perform measurements of magnetic fields in young stars using high-resolution IR
spectroscopy through the Zeeman effect. These observations allow us to
understand how magnetic fields affect the surface and internal structure of young
stars. Direct observations of magnetic fields and stellar properties also permit us to
study the origin of magnetism in stars.
I study the physical properties of young stars using a combination of infrared
spectroscopy and (sub)-mm observations. By measuring key stellar properties
such as mass, age, and accretion, we can learn how young stars grow and
evolve.
Furthermore, I study the physical properties of protoplanetary disks through (sub)mm ALMA
observations. By characterizing the amount of material in the disks, we can
understand how much mass is available for planet formation and for further stellar
growth. Characterizing the gas kinematics of disks is also a fundamental way of
measuring stellar masses and testing theoretical stellar models.