Results 81 to 90 of about 3,519 (205)
Methanol Ice in the Protostar GL 2136 [PDF]
We present ground-based spectra in the 10 and 20 micron atmospheric windows of the deeply embedded protostar GL 2136. These reveal narrow absorption features at 9.7 and 8.9 microns, which we ascribe to the CO-stretch and CH3 rock (respectively) of solid ...
BARLOW, MJ +3 more
core +1 more source
Investigating Protostellar Accretion (IPA) is a JWST Cycle 1 GO program that uses NIRSpec integral field units and MIRI Medium Resolution Spectrograph to obtain 2.9–28 μ m spectral cubes of young, deeply embedded protostars with luminosities of 0.2–10 ...
Mayank Narang +38 more
doaj +1 more source
DISCOVERY OF A MASSIVE PROTOSTAR NEAR IRAS 18507+0121 [PDF]
We have observed the massive star-forming region IRAS 18507+0121 at millimeter wavelengths in 3 mm continuum emission, H13CO+ ( J ¼ 1 0) and SiO (v ¼ 0, J ¼ 2 1) line emission, and at near-infrared (NIR) wavelengths between 1.2 and 2.1 m.
Bronfman Aguiló, Leonardo +2 more
core
Complex Organic Molecules tracing shocks along the outflow cavity in the high-mass protostar IRAS 20126+4104 [PDF]
We report on subarcsecond observations of complex organic molecules (COMs) in the high-mass protostar IRAS 20126+4104 with the Plateau de Bure Interferometer in its most extended configurations. In addition to the simple molecules SO, HNCO and H₂¹³CO, we
Cesaroni, R +26 more
core +1 more source
WARPfold : Wrongfield ARithmetic for Protostar folding [PDF]
Inspired by range-check trick from recent Latticefold paper we construct elliptic-curve based IVC capable of simulating non-native arithmetic efficiently.
Lev Soukhanov
core
The composition of protoplanetary disks, and hence the initial conditions of planet formation, may be strongly influenced by the infall and thermal processing of material during the protostellar phase.
Himanshu Tyagi +38 more
doaj +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Contents
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S2-S47, August 2026.
wiley +1 more source
The Structure and Kinematics of Three Class 0 Protostellar Jets from JWST
We present observations of jets within 2000 au of three deeply embedded protostars using 2.9–27 μ m observations with JWST. These observations show the morphologies and kinematics of the collimated jets from three protostars, the low-mass Class 0 ...
Samuel A. Federman +22 more
doaj +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source
Water and methanol are key components of interstellar ices and gas in star- and planet-forming regions, but direct observations of water in low-mass protostars are challenging due to atmospheric absorption.
Curtis DeWitt +10 more
doaj +1 more source

