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Disk Masses for Embedded Class I Protostars in the Taurus Molecular Cloud
Patrick D. Sheehan, Josh A. Eisner
Class I protostars are thought to represent an early stage in the lifetime of protoplanetary disks, when they are still embedded in their natal envelope. Here we measure the disk m…
An Explanation of the Very Low Radio Flux of Young Planet-mass Companions
Ya-Lin Wu, Laird M. Close, Josh A. Eisner +1
We report Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum upper limits for 5 planetary-mass companions DH Tau B, CT Cha B, GSC 6214-210 B, 1RXS 1609 B, and GQ…
Improved Constraints on the Disk Around MWC 349A from the 23-Meter LBTI
Steph Sallum, Josh Eisner, Phil Hinz +4
We present new spatially resolved observations of MWC 349A from the Large Binocular Telescope Interferometer (LBTI), a 23-meter baseline interferometer made up of two, co-mounted 8…
WL 17: A Young Embedded Transition Disk
Patrick D. Sheehan, Josh A. Eisner
We present the highest spatial resolution ALMA observations to date of the Class I protostar WL 17 in the Ophiuchus L1688 molecular cloud complex, which show that it has a 12 A…
The ALMA View of the OMC1 Explosion in Orion
John Bally, Adam Ginsburg, Hector Arce +4
Most massive stars form in dense clusters where gravitational interactions with other stars may be common. The two nearest forming massive stars, the BN object and Source I, locate…