ﻻ يوجد ملخص باللغة العربية
High-redshift dusty star-forming galaxies with very high star formation rates (500 -- 3000 M$_odot$ yr$^{-1}$) are key to understanding the formation of the most extreme galaxies in the early Universe. Characterising the gas reservoir of these systems can reveal the driving factor behind the high star formation. Using molecular gas tracers like high-J CO lines, neutral carbon lines and the dust continuum, we can estimate the gas density and radiation field intensity in their interstellar medium. In this paper, we present high resolution($sim$0.4) observations of CO(7-6), [CI](2-1) and dust continuum of 3 lensed galaxies from the SPT-SMG sample at z$sim$3 with the Atacama Large Millimeter/submillimeter Array. Our sources have high intrinsic star-formation rates (>850 M$_odot$ yr$^{-1}$) and rather short depletion timescales (<100 Myr). Based on the $rm L_{[rm CI](2-1)}/ rm L_{rm CO(7-6)}$ and $rm L_{[rm CI](2-1)}/rm L_{rm IR}$ ratios, our sample galaxies exhibit higher radiation field intensity compared to other submillimetre galaxies but have similar gas densities. We perform visibility-based lens modelling on these objects to reconstruct the kinematics in the source plane. We find that the cold gas masses of the sources are compatible with simple dynamical mass estimates using ULIRG-like values of the CO-H$_2$ conversion factor $alpha_{rm CO}$ but not Milky Way-like values. We find diverse source kinematics in our sample: SPT0103-45 and SPT2147-50 are likely rotating disks while SPT2357-51 is a probable major merger. The analysis presented in the paper could be extended to a larger sample to determine better statistics of morphologies and interstellar medium properties of high-z dusty star-forming galaxies.
We present PHANGS-ALMA, the first survey to map CO J=2-1 line emission at ~1 ~ 100pc spatial resolution from a representative sample of 90 nearby (d<~20 Mpc) galaxies that lie on or near the z=0 main sequence of star-forming galaxies. CO line emissio
We have modelled high resolution ALMA imaging of six strong gravitationally lensed galaxies detected by the Herschel Space Observatory. Our modelling recovers mass properties of the lensing galaxies and, by determining magnification factors, intrinsi
The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-forming galaxies (DSFGs) over a wide range in redshift. A detailed understanding of these DSFGs is hampered by the limited spatial resolution of Hersch
We present high-fidelity, 30 milliarcsecond (200-pc) resolution ALMA rest-frame 240 $mu$m observations of cold dust emission in three typical main-sequence star-forming galaxies (SFGs) at $z sim 3$ in the Hubble Ultra-Deep Field (HUDF). The cold dust
The South Pole Telescope has discovered one hundred gravitationally lensed, high-redshift, dusty, star-forming galaxies (DSFGs). We present 0.5 resolution 870um Atacama Large Millimeter/submillimeter Array imaging of a sample of 47 DSFGs spanning z=1