Quantitative Spectroscopy of Photoionized Clouds

By G. Ferland. 2003

153 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics

View Paper: https://www.semanticscholar.org/paper/5eb00e756aa7707dafda8c7be925724df166199c

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. E. Dishoeck
2. E. Bergin
3. K. Oberg
4. A. C. Fabian
5. J. Reeves
6. J. Black
7. Tamás Budavári
8. J. Walcher

In Atomic and Molecular Physics, and Optics

1. E. Bergin
2. K. Oberg
3. J. Black
4. France.
5. The Netherlands.
6. Ralf-Jurgen Dettmar
7. E. Dishoeck
8. J. E. Beckman

Citations in the corpus

• A computer program for fast non-LTE analysis of interstellar line spectra With diagnostic plots to interpret observed line intensity ratios (2007, background): “Freefree radiation may become important for the calculation of atomic fine structure lines from H II regions; other programs such asCLOUDY (Ferland 2003)9 may be more suitable for this purpose.”
• Spectral changes during dipping in low-mass X-ray binaries due to highly-ionized absorbers (2005, methodology): “In this paper, we use a grid of ionic column densities pre-calculated using CLOUDY and assuming that the ionizing continuum for each source may be represented by a cutoff power-law (E−Γ exp (−E/Ec)) with a power-law index, Γ, obtained from the fits to the EPIC pn persistent spectra with the cutoff e”
• Diffuse Atomic and Molecular Clouds (2006, methodology): “An emerging development in this field is the recent application of the workhorse spectral synthesis code Cloudy (reviewed in Ferland 2003) to diffuse clouds.”
• The warm ionized medium in spiral galaxies (2009, methodology): “ state within the emitting gas. For many years, these diagnostic techniques have been applied to a variety of astrophysical plasmas (see, e.g., Davidson and Netzer, 1979; Dopita and Sutherland, 2003; Ferland, 2003; Osterbrock, 1989; Osterbrock and Ferland, 2006, for in depth discussions), but only m”
• Collisional heating as the origin of filament emission in galaxy clusters (2008, background): “Their intensity ratio has no direct dependence on the abundances (Ferland 2003).”
• EVIDENCE FOR ULTRA-FAST OUTFLOWS IN RADIO-QUIET ACTIVE GALACTIC NUCLEI. II. DETAILED PHOTOIONIZATION MODELING OF Fe K-SHELL ABSORPTION LINES (2011, methodology): “In particular, they derived the iron ions populations using a different photo-ionization code, CLOUDY (Ferland 2003), but considered the same power-law continuum with Γ=2 as in this work.”
• Photodissociation and photoionisation of atoms and molecules of astrophysical interest (2017, background): “…have long been an object of theoretical study due to their influence on the interpretation of spectroscopic observations of astrophysical plasmas in ionised interstellar gas as found around stars, active galactic nuclei, and elsewhere (Seaton 1951; Osterbrock 1979; Ferland 2003; Tielens 2013).”
• Astrochemistry and compositions of planetary systems (2020, background): “Phototionization of H and other atoms, and its balance with recombination is reviewed by Ferland (2003).”
• Fitting the integrated spectral energy distributions of galaxies (2010, background): “For further details, see reviews by Ferland (2003) and Stasińska (2007).”