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]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
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]

open access: yesAstronomy and Astrophysics
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]

open access: yesAstrophysical Journal, 2015
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]

open access: yesAstrophysical Journal, 2020
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]

open access: yesAstronomy & Astrophysics
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 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
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

Predictions of Dust Continuum Emission from a Potential Circumplanetary Disk: A Case Study of the Planet Candidate AB Aurigae b

open access: yesAstrophysical Journal
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]

open access: yesAstronomy & Astrophysics, 2002
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

Constraints on PDS 70 b and c from the dust continuum emission of the circumplanetary discs considering in situ dust evolution

open access: yesAstronomy & Astrophysics
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

open access: yes
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

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