Results 101 to 110 of about 4,978 (213)
The Protostars in Orion: Characterizing the Properties of Their Magnetized Envelopes
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
IPA: Class 0 Protostars Viewed in CO Emission Using JWST
We investigate the bright CO fundamental emission in the central regions of five protostars in their primary mass assembly phase using new observations from JWST’s Near-Infrared Spectrograph and Mid-Infrared Instrument. CO line emission images and fluxes
Adam E. Rubinstein +26 more
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Proceedings of Protostars and Planets V
Oral presentation sessions in this conference include: Clouds and cores; Star formation and protostars; Binaries and multiples; Newborn massive stars; jets and outflows; Clusters and associations; T Tauri stars and disks; Brown dwarfs; Planet formation ...
core
Effect of Magnetic Field on the Accretion Phase of Population III Star Formation
We examine the impact of the magnetic field on Population III star formation by varying its strength. We perform simulations with magnetic field strengths ranging from 10 ^−20 G to 10 ^−4 G, in addition to a model without a magnetic field.
Masahiro N. Machida +2 more
doaj +1 more source
Protostellar outflows and jets are almost ubiquitous characteristics during the mass accretion phase and encode the history of stellar accretion, complex organic molecule (COM) formation, and planet formation.
Somnath Dutta +24 more
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Nascent Embedded-protostar Survey in Taurus (NEST). I. Protostellar Multiplicity
We present new Atacama Large Millimeter/submillimeter Array (ALMA) 0.9 mm and Very Large Array (VLA) 9 mm observations in the Taurus Molecular Cloud (TMC) of 25 protostellar systems, containing 40 protostars, observed at 0 $\mathop{.}\limits^{^{\prime ...
Aislinn C. Plante +7 more
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Identification of solid N2O in interstellar ices using open JWST data
Context. Only six molecules containing an N-O bond are detected in the gaseous phase of the interstellar medium. One of them is nitrous oxide (N2O), which was unsuccessfully searched for in solid form since the launch of the Infrared Space Observatory ...
Karteyeva V. +4 more
doaj +1 more source
A Comparison of Presolar Isotopic Signatures in Laboratory-Studied Primitive Solar System Materials and Comet 67P/Churyumov-Gerasimenko: New Insights from Light Elements, Halogens, and Noble Gases. [PDF]
Hoppe P, Rubin M, Altwegg K.
europepmc +1 more source
First Detection of CH3OD in Prestellar Cores
The isotopic ratios of deuterated methanol derived around protostars are commonly used to infer the physical conditions under which they formed in the earlier prestellar stage.
Beatrice M. Kulterer +8 more
doaj +1 more source
Outflows from the youngest stars are mostly molecular. [PDF]
Ray TP +22 more
europepmc +1 more source

