Results 101 to 110 of about 13,657 (239)
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
Episodic accretion, radiative feedback, and their role in low-mass star formation
It is speculated that the accretion of material onto young protostars is episodic. We present a computational method to include the effects of episodic accretion in radiation hydrodynamic simulations of star formation.
Hubber, David +2 more
core
Thermal structure of a protostellar envelope
A numerical hydrodynamical model for the evolution of spherically symmetric collapsing clouds, designed for the calculation of the thermal structure of these objects in both the prestellar and protostellar stages of their evolution, is presented ...
Fateeva, A. M. +3 more
core +1 more source
SUBARCSECOND ANALYSIS OF THE INFALLING–ROTATING ENVELOPE AROUND THE CLASS I PROTOSTAR IRAS 04365+2535 [PDF]
Nami Sakai +12 more
openalex +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
A "Starless" Core that Isn't: Detection of a Source in the L1014 Dense Core with the Spitzer Space Telescope [PDF]
We present observations of L1014, a dense core in the Cygnus region previously thought to be starless, but data from the Spitzer Space Telescope show the presence of an embedded source. We propose a model for this source that includes a cold core, heated
Blake, Geoffrey A. +4 more
core
Optical spectroscopy of Gaia detected protostars with DOT: can we probe protostellar photospheres? [PDF]
Mayank Narang +9 more
openalex +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
Pre- and Post-burst Radio Observations of the Class 0 Protostar HOPS 383\n in Orion [PDF]
Roberto Galván-Madrid +7 more
openalex +1 more source

