Results 91 to 100 of about 3,519 (205)
Infall and outflow within 400 AU from a high-mass protostar
Observational signatures of infalling envelopes and outflowing material in early stages of protostellar evolution and at small radii from the protostar are essential to progress in the understanding of the mass-accretion process in star formation.
L. Moscadelli, A. Sanna, C. Goddi
core +1 more source
Star formation is a fundamental, yet poorly understood, process of the Universe. It is important to study how star formation occurs in different galactic environments.
Yu Cheng +7 more
doaj +1 more source
Evidence for a bloated massive protostar in IRAS 20126+4104
Context. Variability is a well-known phenomenon in low-mass young stellar objects, but in recent years the monitoring of methanol masers and IR continuum emission has permitted the detection of both burst-like episodes and periodic variations in high ...
Cesaroni R.
doaj +1 more source
We present high-resolution (∼0 $\mathop{.}\limits^{^{\prime\prime} }$ 05; 8 au) dust continuum and molecular line observations toward the Class I protostellar system IRAS 04169+2702 in the Taurus B213 region, as part of the Atacama Large Millimeter ...
Ilseung Han +24 more
doaj +1 more source
Twisted Pseudodisk and Asymmetric Mass Accretion on the Circumstellar Disk
We model gas inflow patterns onto circumstellar disks and the evolution of the pseudodisk using three-dimensional resistive MHD simulations. Starting from a prestellar core without turbulence and with a misalignment between the initial magnetic field and
Masahiro N. Machida +2 more
doaj +1 more source
Gamma-rays from massive protostars
Fil: Paredes, Josep Maria. Universidad de Barcelona.
Romero, Gustavo Esteban +3 more
openaire +5 more sources
First Detection of Circular Polarization in Radio Continuum Toward a Massive Protostar
Polarization measurements provide strong constraints on magnetic fields in star-forming systems. While magnetic field estimates of a few kG have been obtained near the surfaces of low-mass protostars, there are no analogous measurements in the immediate ...
A. G. Cheriyan +6 more
doaj +1 more source
While molecular outflows have been studied in detail with radio interferometry, observations of the hotter gas in protostellar outflows at a comparable physical scale are often challenging.
Yuki Okoda +12 more
doaj +1 more source
Deuterium fractionation in the closest vicinity of a protostar is important in understanding its potential heritage to a planetary system. Here, we have detected the spectral line emission of CH _3 OH and its three deuterated species, CH _2 DOH, CHD _2 ...
Yuki Okoda +7 more
doaj +1 more source
Outflows from the youngest stars are mostly molecular. [PDF]
Ray TP +22 more
europepmc +1 more source

