My research focuses on the physics and chemistry of low-mass young stellar objects (YSOs) using data on high-
J CO obtained by
the Herschel Guaranteed Time Key Project,
WISH "Water in
Star-forming regions with
Herschel" (PI:
Ewine van Dishoeck) together with observations from JCMT and APEX.
Most studies concentrated on the cold gas and dust -as probed by low-
J CO lines (J≤3)-, however, in my research,
we follow the warm gas -as probed by higher-
J CO lines (J≥6)- which is much more diagnostic of the energetic
processes that shape these deeply embedded sources. Our main question is, the quantification and location of the gas
that is heated in the envelope via various processes. In addition, the abundance structure of CO is investigated.
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Where does Earth's water come from?
I was Teaching Assistant for
Stellar Structure and Evolution Lecture in Spring 2010.
Happy 400th year of Dutch-Turkish diplomatic relations celebrations
