Results 101 to 110 of about 3,519 (205)
FAUST. XIV. Probing the Flared Disk in L1527 with Sulfur-bearing Molecules
IRAS04368+2557 in L1527 is a Class 0/I protostar with a clear disk-envelope system revealed by previous Atacama Large Millimeter/submillimeter Array (ALMA) observations.
Ziwei E. Zhang +23 more
doaj +1 more source
Observations of a High-mass Protostar in Ngc 7538 S
We present high angular resolution continuum observations of the high-mass protostar NGC 7538 S with BIMA and CARMA at 3 and 1.4 mm, Very Large Array (VLA) observations at 1.3, 2, 3.5, and 6 cm, and archive Infrared Array Camera (IRAC) observations from ...
Zhu, Lei +5 more
core +1 more source
We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the Class 0 protostar IRAS 04166+2706, obtained as part of the ALMA Large Program Early Planet Formation in Embedded Disks.
Nguyen Thi Phuong +22 more
doaj +1 more source
Context. The physical conditions within the innermost few tens of astronomical units of high-mass protostars (M* > 8 M⊙) remain largely unexplored.
Fedriani R. +9 more
doaj +1 more source
DISK-OUTFLOW SYSTEM AROUND A MASSIVE PROTOSTAR
Author Institution: Department of Astronomy, University of Illinois, 1002 W. Grenn St., Urb; ana, IL 61801; Department of Astronomy, University of Wisconsin at Madison, 475 North; Charter St., Madison, WI 53705There are two major competing models for ...
Churchwell, E., Kim, Kee-Tae
core
Disk-mediated accretion is central to theories of massive star formation, setting the initial conditions for their evolution. Yet observations of Keplerian disks around early O-type protostars remain scarce, as they are often blended into complex ...
Jixiang Weng +24 more
doaj +1 more source
The MATISSE view of the inner region of the RY Tau protoplanetary disk★
Context. The physical conditions and processes taking place in the innermost regions of protoplanetary disks are essential for planet formation and general disk evolution.
Martin J. S. +46 more
doaj +1 more source
The Extent of Solar Energetic Particle Irradiation in the Sun’s Protoplanetary Disk
Solar flares emit X-rays and high-energy (MeV to GeV) ions called solar energetic particles (SEPs). Astronomical observations show solar-mass protostellar fluxes are a factor Φ ≈ 3 × 10 ^2 –3 × 10 ^3 times higher than the present-day Sun.
Steven J. Desch +3 more
doaj +1 more source
Multiple Jets in the Bursting Protostar HOPS 373SW
We present the outflows detected in HOPS 373SW, a protostar undergoing a modest 30% brightness increase at 850 μ m. Atacama Large Millimeter/submillimeter Array observations of shock tracers, including SiO 8–7, CH _3 OH 7 _k –6 _k , and ^12 CO 3–2 ...
Seokho Lee +4 more
doaj +1 more source
Overmassive black holes and little red dots naturally form in simulations. [PDF]
Chon S +4 more
europepmc +1 more source

