Results 71 to 80 of about 1,150 (163)
Fast, collimated jets are ubiquitous features of young stellar objects. They are generally thought to be powered by disk accretion, but the details are debated.
Yisheng Tu +4 more
doaj +1 more source
ERRATUM: "YOUNG STELLAR OBJECTS IN THE MASSIVE STAR FORMING REGION W49". [PDF]
Saral G +5 more
europepmc +1 more source
Radio Continuum and Water Maser Observations of the High-mass Protostar IRAS 19035+0641 A
We present Very Large Array 1.3 cm continuum and 22.2 GHz H _2 O maser observations of the high-mass protostellar object IRAS 19035+0641 A. Our observations unveil an elongated bipolar 1.3 cm continuum structure at scales ≲500 au, which, together with a ...
Tatiana M. Rodríguez +4 more
doaj +1 more source
YOUNG STELLAR OBJECTS IN THE MASSIVE STAR-FORMING REGION W49. [PDF]
Saral G +5 more
europepmc +1 more source
Young Stellar Objects In Orion B
I will discuss our search for young stellar objects in the northern part of the Orion molecular cloud B, where we identify almost 200 young stellar objects that coincide or are located close to sites of active star formation. With the total gas mass of the cloud substructures, we calculate local star formation efficiencies, rates, and the star ...
openaire +1 more source
Iron inclusions embedded inside dust grains play a crucial role in both internal alignment (IA) via Barnett relaxation and external alignment via the MAgnetically Enhanced RAdiative Torque (MRAT) mechanism.
Nguyen Chau Giang +4 more
doaj +1 more source
Dust Polarization of Prestellar and Protostellar Sources in OMC-3
We present the Atacama Large Millimeter/submillimeter Array observations of linearly polarized 1.1 mm continuum emission at ∼0.″14 (55 au) resolution and CO ( J = 2−1) emission at ∼1.″5 (590 au) resolution toward one prestellar (MMS 4), four Class 0 (MMS
Yuhua Liu +7 more
doaj +1 more source
ABYSS. II. Identification of Young Stars in Optical SDSS Spectra and Their Properties
We developed a tool that measures equivalent widths of various lines in low-resolution optical spectra, and it was applied to stellar spectra obtained as part of SDSS-V and LAMOST programs.
Serat Saad +11 more
doaj +1 more source
Spectroscopic constraints on CH3OH formation: CO mixed with CH3OH ices towards young stellar objects. [PDF]
Penteado EM +5 more
europepmc +1 more source

