Results 1 to 10 of about 4,700 (187)
ALMA uncovers the [C ii] emission and warm dust continuum in a z = 8.31 Lyman break galaxy [PDF]
We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA).
Hashimoto, Takuya +53 more
core +7 more sources
Bayesian analysis of the molecular emission and dust continuum of protoplanetary disks [PDF]
Context. The MIRI instrument on board the James Webb Space Telescope probes the chemistry and dust mineralogy of the inner regions of protoplanetary disks.
Arabhavi, A. M.; id_orcid +11 more
core +5 more sources
Dust Continuum Emission as a Tracer of Gas Mass in Galaxies [PDF]
The authors thank the anonymous referee whose comments helped expand and improve the details of this work. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated ...
Galametz, Maud +10 more
core +7 more sources
Kiloparsec-scale ALMA imaging of [C ii] and dust continuum emission of 27 quasar host galaxies at z ~ 6 [PDF]
We present a study of the [CII] 158micron line and underlying far-infrared (FIR) continuum emission of 27 quasar host galaxies at z~6, traced by the Atacama Large Millimeter/submillimeter Array at a spatial resolution of ~1 physical kpc.
Rix, H. +29 more
core +8 more sources
ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion [PDF]
Context. Low- and intermediate-mass stars on the asymptotic giant branch (AGB) account for a significant portion of the dust and chemical enrichment in their host galaxy.
Wong, KT +37 more
core +10 more sources
Predictions for the spatial distribution of the dust continuum emission in 1
We present the first detailed study of the spatially resolved dust continuum emission of simulated galaxies at 1 < z < 5. We run the radiative transfer code skirt on a sample of submillimetre-bright galaxies drawn from the Feedback In Realistic ...
Lotz, J +9 more
core +6 more sources
Gas-accreting planets embedded in protoplanetary disks are expected to show dust thermal emission from their circumplanetary disks (CPDs). However, a recently reported gas-accreting planet candidate, AB Aurigae b, has not been detected in (sub)millimeter
Yuhito Shibaike +5 more
core +3 more sources
Probing the mass loss history of carbon stars using CO line and dust continuum emission [PDF]
An extensive modelling of CO line emission from the circumstellar envelopes around a number of carbon stars is performed. By combining radio observations and infrared observations obtained by ISO the circumstellar envelope characteristics are ...
H. Olofsson +5 more
core +4 more sources
Context. The young T Tauri star PDS 70 has two gas accreting planets sharing one large gap in a pre-transitional disc. Dust continuum emission from PDS 70 c has been detected by Atacama Large Millimeter/submillimeter Array (ALMA) Band 7, considered as ...
Y. Shibaike +3 more
core +2 more sources
Modeling the dust continuum emission from protoplanetary disks
We modeled the dust continuum emission from the protoplanetary disk of the protostar GM Aurigae (GM Aur) using publicly available software DiskMINT and RADMC-3D. We also incorporated and investigated the effect of magnetic winds on this emission.
Syed Hassaan Azam
core +2 more sources

