Results 11 to 20 of about 3,519 (205)

The Outflow of The Protostar in B335. I. [PDF]

open access: yesThe Astronomical Journal
The isolated globule B335 contains a single, low-luminosity Class 0 protostar associated with a bipolar nebula and outflow system seen nearly perpendicular to its axis.
Klaus W. Hodapp   +12 more
doaj   +6 more sources

An Outbursting Protostar: The Environment of L1251 VLA 6 [PDF]

open access: yesThe Astrophysical Journal
Young protostars that undergo episodic accretion can provide insight into the impact on their circumstellar environments while matter is accreted from the disk onto the protostar.
Ava Nederlander   +8 more
doaj   +4 more sources

Multiple Outflows around a Single Protostar IRAS 15398−3359

open access: yesThe Astrophysical Journal
We present the results of our mosaic observations of a single Class 0 protostar IRAS 15398−3359 with the Atacama Compact Array in the CO J = 2–1 line.
Jinshi Sai   +6 more
doaj   +2 more sources

The Agn As A Protostar

open access: yes, 2017
AGN - Protostar ...
Elitzur Moshe (5297176), Elitzur Moshe
openaire   +3 more sources

Connecting a Magnetized Disk to a Convective Low-mass Protostar: A Global 3D Model of Boundary Layer Accretion [PDF]

open access: yesThe Astrophysical Journal
In the early stages of star formation, boundary layer accretion, where protostars accrete material from disks extending down to their surfaces, plays a crucial role.
Shinsuke Takasao   +3 more
doaj   +2 more sources

IPA: Accretion Rate of a Low-mass Class 0 Protostar, Measured via Mid-IR Fluorescent OH Emission

open access: yesThe Astrophysical Journal
The earliest stages of star formation are highlighted by complex interactions between accretion, outflow, and radiative processes, which shape the chemical and physical environment of the emerging protostar. James Webb Space Telescope observations of the
Dan M. Watson   +43 more
doaj   +2 more sources

ORPHANED PROTOSTARS [PDF]

open access: yesThe Astrophysical Journal, 2010
We explore the origin of a population of distant companions (~1000 - 5000 AU) to Class I protostellar sources recently found by Connelley and co-workers, who noted that the companion fraction diminished as the sources evolved. Here we present N-body simulations of unstable triple systems embedded in dense cloud cores.
Reipurth, Bo   +3 more
openaire   +2 more sources

The Role of Benzonitrile Chlorination Explored by Dissociative Electron Attachment. [PDF]

open access: yesChemphyschem
Experimental and theoretical dissociative electron attachment study of 2‐ and 4‐chlorobenzonitrile. The dissociative electron attachment process to ortho‐ and para‐chlorobenzonitrile was investigated in the 0–12 eV energy range with a crossed‐beam time‐of‐flight mass spectrometer, supported by quantum chemical scattering calculations.
Guerra P   +5 more
europepmc   +2 more sources

Identification of A Collapsing Protostar [PDF]

open access: yesAstrophysics and Space Science, 1994
The globular molecular cloud B335 contains a single, deeply embedded, far-infrared source. Our recent observations of H2CO and CS lines toward this source provide direct kinematic evidence for collapse. Both the intensity and detailed shape of the line profiles match those expected from inside-out collapse inside a radius of 0.036 pc.
Neal J. Evans   +3 more
openaire   +1 more source

CO in Protostars (COPS): Herschel-SPIRE Spectroscopy of Embedded Protostars∗ [PDF]

open access: yesThe Astrophysical Journal, 2018
Abstract We present full spectral scans from 200 to 670 μm of 26 Class 0+I protostellar sources obtained with Herschel-SPIRE as part of the “COPS-SPIRE” Open Time program, complementary to the DIGIT and WISH Key Programs. Based on our nearly continuous, line-free spectra from 200 to 670 μm, the calculated bolometric luminosities (L
Yao-Lun Yang   +15 more
openaire   +8 more sources

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