Results 91 to 100 of about 25,326 (243)

Tracking Star-forming Cores as Mass Reservoirs in Clustered and Isolated Regions Using Numerical Passive Tracer Particles

open access: yesThe Astrophysical Journal
Understanding the physical properties of star-forming cores as mass reservoirs for protostars and the impact of turbulence is crucial in star formation studies.
Shingo Nozaki   +3 more
doaj   +1 more source

The infrared Galactic disk: What have we learned?

open access: yesEPJ Web of Conferences, 2012
A brief overview is given of some of the new insights we have achieved from the Spitzer/GLIMPSE/MIPSGAL surveys of the Galactic plane. Particular emphasis is given to infrared bubbles, rapidly accreting protostars, infrared dark clouds, and diffuse PAH ...
Churchwell E.
doaj   +1 more source

Disk Wind Feedback from High-mass Protostars. IV. Shock-ionized Jets

open access: yesThe Astrophysical Journal
Massive protostars launch accretion-powered, magnetically collimated outflows, which play crucial roles in the dynamics and diagnostics of the star formation process. Here we calculate the shock heating and resulting free–free radio emission in numerical
Emiko C. Gardiner   +5 more
doaj   +1 more source

ngVLA Synthetic Observations of Ionized Gas in Massive Protostars

open access: yesThe Astrophysical Journal
Massive-star formation involves significant ionization in the innermost regions near the central object, such as gravitationally trapped H ii regions, jets, ionized disks, or winds. Resolved observations of the associated continuum and recombination line
Jesús M. Jáquez-Domínguez   +13 more
doaj   +1 more source

Disk Wind Feedback from High-mass Protostars. II. The Evolutionary Sequence [PDF]

open access: gold, 2023
Jan E. Staff   +4 more
openalex   +1 more source

Protostellar Disk Formation Regimes: Angular Momentum Conservation versus Magnetic Braking

open access: yesThe Astrophysical Journal Letters
Protostellar disks around young protostars exhibit diverse properties, with their radii ranging from less than ten to several hundred astronomical units.
Hsi-Wei Yen, Yueh-Ning Lee
doaj   +1 more source

SUBARCSECOND ANALYSIS OF THE INFALLING–ROTATING ENVELOPE AROUND THE CLASS I PROTOSTAR IRAS 04365+2535 [PDF]

open access: bronze, 2016
Nami Sakai   +12 more
openalex   +1 more source

Disk Structure around the Class I Protostar L1489 IRS Revealed by ALMA: A Warped-disk System [PDF]

open access: bronze, 2020
Jinshi Sai   +11 more
openalex   +1 more source

Luminosity Functions of Spitzer Identified Protostars in Nine Nearby Molecular Clouds

open access: yes, 2012
We identify protostars in Spitzer surveys of nine star-forming molecular clouds within 1 kpc: Serpens, Perseus, Ophiuchus, Chamaeleon, Lupus, Taurus, Orion, Cep OB3, and Mon R2, which combined host over 700 protostar candidates.
Allen   +61 more
core   +1 more source

The Protostars in Orion: Characterizing the Properties of Their Magnetized Envelopes

open access: yesThe Astrophysical Journal
We present a study connecting the physical properties of protostellar envelopes to the morphology of the envelope-scale magnetic field. We used the Atacama Large Millimeter/submillimeter Array (ALMA) polarization observations of 61 young protostars at 0 ...
Bo Huang   +19 more
doaj   +1 more source

Home - About - Disclaimer - Privacy