Massive star formation in galaxies: radiative transfer models of the UV to millimetre emission of starburst galaxies

By A. Efstathiou, M. Rowan‐Robinson, R. Siebenmorgen. 2000

183 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/baae767bd55155a5adb111f8e8ab8c67954f5964

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. C. Conroy
2. Lisa J. Kewley
3. D. Narayanan
4. L. Hernquist
5. C. Casey
6. B. Groves
7. M. Dopita
8. D. M. Alexander

In Instrumentation

1. Lisa J. Kewley
2. C. Casey
3. B. Groves
4. D. Dale
5. M. Dopita
6. C. Conroy
7. S. Wuyts
8. D. Lutz

Citations in the corpus

• Dusty Star Forming Galaxies at High Redshift (2014, background): “…work in this area, particularly modeling radiative transfer in local starburst populations to generate SEDs (Efstathiou and Rowan-Robinson, 1995; Efstathiou et al., 2000; Efstathiou and Rowan-Robinson, 2003; Efstathiou and Siebenmorgen, 2009; Nenkova et al., 2002; Dullemond and van Bemmel,…”
• The Dust Opacity of Star‐forming Galaxies (2001, background): “Neverthless, the number counts at mid– and far–IR wavelengths are about 3–10 times above the no-evolution extrapolation of the local IRAS counts (Elbaz et al. 1999; Aussel et al. 1999; Puget et al. 1999; Serjeant et al. 2000; Efstathiou et al. 2000).”
• Fitting the integrated spectral energy distributions of galaxies (2010, methodology): “The models of Efstathiou et al. (2000) and Siebenmorgen and Krügel (2007) do this radiative-transfer calculation using the ray-tracing method for starburst galaxies, which, being dominated by young stars and their birth clouds, are well represented by simple spherical approximations.”
• Dust in starburst nuclei and ULIRGs - SED models for observers (2006, result): “This is also reflected by the controversial interpretations via an old stellar population (Silva et al. 1998) or via young, but obscured stars (Efstathiou et al. 2000).”
• Modelling the spectral energy distribution of galaxies - V. The dust and PAH emission SEDs of disk galaxies (2010, background): “Models for starburst galaxies can befound in Rowan-Robinson & Efstathiou 1993, Krügel & Siebenmorgen 1994, Silva et al. 1998, Efstathiou et al. 2000, Takagi et al. 2003,Dopita et al. 2005, Siebenmorgen & Krügel 2007, Groves et al. 2008.”
• Panchromatic spectral energy distributions of Herschel sources (2013, methodology): “…(UV) to FIR, making use of radiative transfer and ray tracing techniques (e.g. Siebenmorgen & Krügel 2007; Piovan et al. 2006; Dopita et al. 2005; Efstathiou et al. 2000; Silva et al. 1998), provides extensive information on the physical properties of star-forming regions, molecular clouds,and…”
• THE COSMIC INFRARED BACKGROUND: Measurements and Implications ⁄ (2001, background): “…1996; Devriendt et al 1999), to more complex models consisting of a clumpy distribution of absorbers, and a mix of uniformly distributed and partially embedded sources (Witt & Gordon 1996; Silva et al 1998; Városi & Dwek 1999; Devriendt et al 1999; Misselt et al 2001; Efstathiou et al 2000).”
• Modeling the Pan-Spectral Energy Distribution of Starburst Galaxies. IV. The Controlling Parameters of the Starburst SED (2007, methodology): “Associated with the latter models is the approach by Efstathiou et al. (2000).”
• Radio Properties of Infrared-selected Galaxies in the IRAS 2 Jy Sample (2001, methodology): “To quantify this trend, the color evolution track for a starburst galaxy com puted by Efstathiou et al. (2000) is shown as a thick curve in Figure 10.”