Add to ORKGv.499 of this Conference Series entitled: Revolution in Astronomy with ALMA: The Third YearWe present our ALMA Cycle 0 result of a protostellar binary system L1551 NE, and discuss our future Cycle 2 observation
ALMA cycles 1 and 3 observations of CO isotopologues and 1.3mm continuum are used in a study of the ...
We present VLA and ALMA observations of the close (0.3" = 90 au separation) protobinary system SVS 1...
Recent theoretical models indicate that OB-type stars could form through disk-mediated accretion, li...
We will report our latest ALMA results of the Class I protostellar binaries L1551 IRS 5, L1551 NE, a...
We report the ALMA observation of the Class I binary protostellar system L1551 NE in the 0.9-mm cont...
Most solar-type stars are created in multiple star systems. One of the effects of how the presence o...
L1551 IRS 5 is a FUor-like object located in the Taurus star-forming region. We present Atacama Larg...
International audienceScattered light high-resolution imaging of the protoplanetary disc orbiting HD...
ABSTRACT Scattered light high-resolution imaging of the protoplanetary disc orbiting ...
We present ALMA observations of a wide binary system in Orion, with projected separation 440 AU, in ...
Aims. We study the circumstellar evolution of the binary HD 101584, consisting of a post-AGB star an...
International audienceWe present Very Large Array (VLA) and Atacama Large Millimeter/submillimeter A...
Aims. We study the circumstellar evolution of the binary HD 101584, consisting of a post-AGB star an...
Thanks to the exquisite high spatial resolution afforded by instruments such as SPHERE and ALMA we c...
We present an observation of L1551 IRS 5 at 7 mm with an angular resolution as high as ∼0″.04 (5 AU)...
ALMA cycles 1 and 3 observations of CO isotopologues and 1.3mm continuum are used in a study of the ...
We present VLA and ALMA observations of the close (0.3" = 90 au separation) protobinary system SVS 1...
Recent theoretical models indicate that OB-type stars could form through disk-mediated accretion, li...
We will report our latest ALMA results of the Class I protostellar binaries L1551 IRS 5, L1551 NE, a...
We report the ALMA observation of the Class I binary protostellar system L1551 NE in the 0.9-mm cont...
Most solar-type stars are created in multiple star systems. One of the effects of how the presence o...
L1551 IRS 5 is a FUor-like object located in the Taurus star-forming region. We present Atacama Larg...
International audienceScattered light high-resolution imaging of the protoplanetary disc orbiting HD...
ABSTRACT Scattered light high-resolution imaging of the protoplanetary disc orbiting ...
We present ALMA observations of a wide binary system in Orion, with projected separation 440 AU, in ...
Aims. We study the circumstellar evolution of the binary HD 101584, consisting of a post-AGB star an...
International audienceWe present Very Large Array (VLA) and Atacama Large Millimeter/submillimeter A...
Aims. We study the circumstellar evolution of the binary HD 101584, consisting of a post-AGB star an...
Thanks to the exquisite high spatial resolution afforded by instruments such as SPHERE and ALMA we c...
We present an observation of L1551 IRS 5 at 7 mm with an angular resolution as high as ∼0″.04 (5 AU)...
ALMA cycles 1 and 3 observations of CO isotopologues and 1.3mm continuum are used in a study of the ...
We present VLA and ALMA observations of the close (0.3" = 90 au separation) protobinary system SVS 1...
Recent theoretical models indicate that OB-type stars could form through disk-mediated accretion, li...