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Open AccessJournal Article

The 2017 release of CLOUDY

TLDR
The 2017 version of Cloudy as mentioned in this paper is the most recent version of the spectral synthesis code, which has made many improvements to the scope and accuracy of the physics which have been made since the previous release.
Abstract
We describe the 2017 release of the spectral synthesis code Cloudy , summa- rizing the many improvements to the scope and accuracy of the physics which have been made since the previous release. Exporting the atomic data into external data files has enabled many new large datasets to be incorporated into the code. The use of the complete datasets is not realistic for most calculations, so we describe the lim- ited subset of data used by default, which predicts significantly more lines than the previous release of Cloudy . This version is nevertheless faster than the previous release, as a result of code optimizations. We give examples of the accuracy limits using small models, and the performance requirements of large complete models. We summarize several advances in the H- and He-like iso-electronic sequences and use our complete collisional-radiative models to establish the densities where the coronal and local thermodynamic equilibrium approximations work.

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Posted Content

The IllustrisTNG Simulations: Public Data Release

TL;DR: Improvements and new functionality in the web-based API are described, including on-demand visualization and analysis of galaxies and halos, exploratory plotting of scaling relations and other relationships between galactic and halo properties, and a new JupyterLab interface that provides an online, browser-based, near-native data analysis platform enabling user computation with local access to TNG data, alleviating the need to download large datasets.
Journal ArticleDOI

Inferring the star formation histories of massive quiescent galaxies with BAGPIPES: evidence for multiple quenching mechanisms

TL;DR: Bayesian Analysis of Galaxies for Physical Inference and Parameter EStimation (BAGPIPES) as discussed by the authors is a new Python tool which can be used to rapidly generate complex model galaxy spectra and to fit these to arbitrary combinations of spectroscopic and photometric data using the MultiNest nested sampling algorithm.
Journal ArticleDOI

The [CII] 158 μm line emission in high-redshift galaxies

TL;DR: In this paper, a semi-analytical model of galaxy evolution combined with the photoionisation code CLOUDY was used to predict the [CII] luminosity of a large number of galaxies (25,000 at z ≃ 5) at 4 ≤ z ≤ 8.
Journal ArticleDOI

Accretion of a giant planet onto a white dwarf star

TL;DR: Optical spectroscopy of a hot white dwarf, WD J091405.30+191412, reveals that the chemical abundances in its disk are similar to those thought to exist deep in icy giant planets, so the white dwarf must be accreting a giant planet.
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Book

Astrophysics of Gaseous Nebulae and Active Galactic Nuclei

TL;DR: In this paper, a comparison of theory with observations internal dynamics of gaseous nebulae interstellar dust H II regions in the galactic context is presented. But the results are limited to the case of active galactic nuclei.

Atomic Data and Nuclear Data Tables

TL;DR: In this paper, the ab initio quasirelativistic Hartree-Fock method developed specifically for the calculation of spectral parameters of heavy atoms and highly charged ions is used to derive transition data for a multicharged tungsten ion.
Book ChapterDOI

Introduction to the Study

Abstract: Various coastal settings like beaches, spit and barriers, deltas, estuaries, lagoons, dunes, red dunes, coral reefs, marshes/mangroves, rocky shore, beach rocks, etc. are incorporated with 7516 km lengthy Indian coast. These coastal morphological units have been developed at different time scale. Coastal setting is undergoing uninterrupted alterations through terrestrial and marine systems. Hence the study regarding coastal environments are gaining momentum among planners, administrators and scientists for better management of the coastal zone. The present studied coast i.e. Balasore coast is characterized by the low lying unconsolidated alluviums surface, extended from Udaipur in the north-east to Rasalpur-I in the south-west which is mostly covered by the sandy, loamy and silty soil with high water retention capacity and this part is also drained by mainly three rivers (Subarnarekha, Dugdugi and Burahbolong). The presence of these fluvial impacts may causes the coastal morphodynamic processes of these areas are very multifaceted in nature. Mobilization of sediment endow with the time-dependent amalgamation apparatus by which this morphologic modification occurs. Morphological changes over time always depend on the nature of fluid dynamics and sediment movement in a particular segment of coastal zone. Progressive adjustment of landscape in turn alters boundary circumstances for the fluid dynamics, which develop to produce further revolutionize in sediment-transport patterns and their depositional yield. Sediment properties and profusion influence the process through their influence upon sediment transport and sediment budgets respectively. This part of the book contains the introduction of shoreline dynamics and beach dynamics and different types of morphological elements and their salient features which have significant importance to modify the coastal region. This introducing sort of the present book is also incorporated with importance of the coastal belt along with the different types of coastal hazard like tropical cyclone, flooding, inundation, storm surges etc. After completion of the study, it also offers some management strategies to formulate the management options for the coastal risk which have frequently kept their worst signatures on geomorphic settings in the coastal environment.
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