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Jets and Disks in Young Stellar Objects Introduction Jets and disks in low-mass young stellar objects The search for jets and disks in massive young stars.
Documents Jets and Disks in Young Stellar Objects Introduction Jets and disks in low-mass young stellar...

Slide 1Jets and Disks in Young Stellar Objects Introduction Jets and disks in low-mass young stellar objects The search for jets and disks in massive young stars Other mechanisms…

Oxygen Isotope Heterogeneity in the Solar System The Molecular Cloud Origin Hypothesis and its Implications for the Chemical Composition of Meteorites.
Documents Oxygen Isotope Heterogeneity in the Solar System The Molecular Cloud Origin Hypothesis and its...

Slide 1 Oxygen Isotope Heterogeneity in the Solar System The Molecular Cloud Origin Hypothesis and its Implications for the Chemical Composition of Meteorites and Planetary…

IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute.
Documents IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very...

Slide 1 IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute to…

Science with continuum data ALMA continuum observations: Physical, chemical properties and evolution of dust, SFR, SED, circumstellar discs, accretion.
Documents Science with continuum data ALMA continuum observations: Physical, chemical properties and evolution...

Science with continuum data ALMA continuum observations: Physical, chemical properties and evolution of dust, SFR, SED, circumstellar discs, accretion discs Effects of dust…

The First Stars and Hypernovae
Documents The First Stars and Hypernovae

The First Stars and Hypernovae K. Nomoto (Univ. of Tokyo) M > 105M:SMS (Super Massive Stars) GR instability Collapse M ~ 300－105M: VMO (Very Massive Objects) Nuclear…

Science with continuum data
Documents Science with continuum data

Science with continuum data ALMA continuum observations: Physical, chemical properties and evolution of dust, SFR, SED, circumstellar discs, accretion discs Effects of dust…

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