We present ALMA observations of 12CO, 13CO, and C18O J=2–1 lines and the 230 GHz continuum for the FU Ori-type object (FUor) V900 Mon (d∼1.5 kpc), for which the accretion burst was triggered between 1953 and 2009. We identified CO emission associated with a molecular bipolar outflow extending up to a ∼104 au scale and a rotating molecular envelope extending over >104 au. The interaction ...
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2020-3-20 · Draft version March 20, 2020 Typeset using LATEX twocolumn style in AASTeX63 ALMA 0.88 mm Survey of Disks around Planetary-mass Companions Ya-Lin Wu,1, Brendan P. Bowler,1 Patrick D. Sheehan,2, ySean M. Andrews,3 Gregory J. Herczeg,4 Adam L. Kraus,1 Luca Ricci,5 David J. Wilner,3 and Zhaohuan Zhu6 1McDonald Observatory and the Department of Astronomy, University …
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ABSTRACT. Using a sample of 67 galaxies from the MeerKAT International GigaHertz Tiered Extragalactic Exploration Survey Early Science data, we study the H i-ba
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2020-1-28 · Astronomy & Astrophysics manuscript no. DGtauB_final c ESO 2020 January 28, 2020 ALMA reveals a large structured disk and nested rotating outflows
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2021-2-22 · For the geometry of the outflow, our default model is two conical emitting regions with ϕ = 30°, which yield an area-covering factor f A = 1 − cos ϕ = 0.13 and a volume factor f V = 2/(3 tan ...
2020-1-3 · The differences, t&ly -tclean, vs. compressional wave velocities. between the transit times of the shaly and clean forma- Use of borehole measurements of compressional and tion for both the compressional and shear waves are plot- shear transit times is described by NationsEX for deter-ted vs. the clay or shale fraction for a sandstone with a ...
Empirical trends in stellar X-ray and radio luminosities suggest that very low mass stars and brown dwarfs should not produce significant radio emission. Defying these expectations, strong non-thermal emission has been observed in some UCDs in the 1−10 GHz range, often attributed to global aurorae. At higher radio frequen- cies, flux due to global aurorae becomes unphysical, and is instead ...
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2021-10-3 · Binary neutron-star mergers (BNSMs) are among the most readily detectable gravitational-wave (GW) sources with LIGO. They are also thought to produce short γ-ray bursts (SGRBs), and kilonovae that are powered by r-process nuclei. Detecting these phenomena simultaneously would provide an unprecedented view of the physics during and after the merger of two compact objects. …
2019-10-21 · The parameter τ(r) is the optical thickness, which is described as κ ext Σ(r)(cos i) −1, where κ ext is the dust opacity, Σ(r) is the dust surface density, and i is the disk inclination angle. Here we adopt Σ( r ) ∝ r −1 based on previous observations of disks for Class II YSOs (e.g., Williams & Cieza 2011 ; Takami et al. 2013 ).
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SoFiA 2 is a fully automated spectral-line source finding pipeline originally intended for the detection of galaxies in large HI data cubes. It is a reimplementation of parts of t
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21CMMC is an efficient Python sampler of the semi-numerical reionization simulation code 21cmFAST (ascl:1102.023) can recover constraints on astrophysical parameters from current or future 21 cm EoR experiments, accommodating a variety of EoR models, as well as priors on individual model parameters and the reionization history.
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Spectral windows spw 0 and spw 2 were devoid of conspicuous line emission and were combined to image the continuum. A single self-calibration loop, setting up CASA task gaincal to average whole scans (option ''solint'' set to ''inf''), provided an improvement in tclean images using Briggs weights with robustness parameter r = 0.0, with a dynamic range (i.e. signal-to-noise ratio ...
