Results 101 to 110 of about 25,277 (239)
Infrared emission from protostars
The Astrophysical Journal, 1985 The emergent spectral energy distribution at infrared to radio wavelengths is calculated for the simplest theoretical construct of a low-mass protostar. It is shown that the emergent spectrum in the infrared is insensitive to the details assumed for the temperature profile as long as allowance is made for a transition from optically thick to optically ...
F. C. Adams, F. H. Shu
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VLT integral field spectroscopy of embedded protostars: using near-infrared emission lines as tracers of accretion and outflow [PDF]
, 2010 C. J. Davis +9 more
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The Astronomical JournalProtostellar 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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Protostars and Outflows in the NGC 7538 IRS 9 Cloud Core [PDF]
, 2005 G. Sandell, W. M. Goss, M. C. H. Wright
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IPA: Class 0 Protostars Viewed in CO Emission Using JWST
The Astrophysical JournalWe 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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CORINOS. II. JWST-MIRI Detection of Warm Molecular Gas from an Embedded, Disk-bearing Protostar
The Astrophysical JournalWe present James Webb Space Telescope (JWST) Mid-InfraRed Instrument (MIRI) observations of warm CO and H _2 O gas in emission toward the low-mass protostar IRAS 15398-3359, observed as part of the CORINOS program.
Colette Salyk +10 more
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Episodic accretion, radiative feedback, and their role in low-mass star formation
, 2011 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
Rotation and X‐Ray Emission from Protostars [PDF]
, 2000 T. Montmerle +3 more
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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]
Space Sci Rev, 2023 Hoppe P, Rubin M, Altwegg K.
europepmc +1 more source
, 2000 In an effort to shed more light on the formation process of binary stars, we have started a program to study multiplicity among nearby low- and intermediate-mass protostars using the OVRO Millimeter Array. Here, we describe the project and present the first results on the protostellar core in the Bok globule CB230 (L1177).
Launhardt, R. +2 more
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