Yusuke Aso

Formation of a keplerian disk in the infalling envelope around l1527 IRS: Transformation from infalling motions to kepler motions

We report Atacama Large Millimeter/submillimeter Array (ALMA) cycle 0 observations of C

ALMA OBSERVATIONS OF INFALLING FLOWS TOWARD THE KEPLERIAN DISK AROUND THE CLASS I PROTOSTAR L1489 IRS

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SIGNS OF EARLY-STAGE DISK GROWTH REVEALED WITH ALMA

O (

SMA and ALMA studies of protoplanetary disk formation around low-mass protostars

J=2-1

ALMA OBSERVATIONS OF THE TRANSITION FROM INFALL MOTION TO KEPLERIAN ROTATION AROUND THE LATE-PHASE PROTOSTAR TMC-1A

), SO (

NO KEPLERIAN DISK >10 AU AROUND THE PROTOSTAR B335: MAGNETIC BRAKING OR YOUNG AGE?

J_N= 6_5-5_4

ALMA Observations of the Protostar L1527 IRS: Probing Details of the Disk and the Envelope Structures

) and 1.3mm dust continuum toward L1527 IRS, a class 0 solar-type protostar surrounded by an infalling and rotating envelope. C

SMA and ALMA Studies of Disk- and Planet Formation around Low-mass Protostars

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The Distinct Evolutionary Nature of Two Class 0 Protostars in Serpens Main SMM4

O emission shows strong redshifted absorption against the bright continuum emission associated with L1527 IRS, strongly suggesting infall motions in the C

ALMA Observations of SMM11 Reveal an Extremely Young Protostar in Serpens Main Cluster

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