a new model for the infrared emission of iras f10214+4724
DESCRIPTION
A new model for the infrared emission of IRAS F10214+4724. Andreas Efstathiou European University Cyprus. Introduction to IRAS F10214+4724. Discovered by Rowan-Robinson et al (1991) Gravitationally lensed by a factor of 10 - 100 Similar to Seyfert 2 galaxies in optical-UV - PowerPoint PPT PresentationTRANSCRIPT
5-9th September 2011 SED2011 conference
A new model for the infrared emission of IRAS F10214+4724
Andreas Efstathiou
European University Cyprus
5-9th September 2011 SED2011 conference
Introduction to IRAS F10214+4724
• Discovered by Rowan-Robinson et al (1991)• Gravitationally lensed by a factor of 10 - 100• Similar to Seyfert 2 galaxies in optical-UV• Large quantity of molecular gas and bright in the
submillimeter• Similar to local ULIRGs?
5-9th September 2011 SED2011 conference
Starburst model of Efstathiou, Rowan-Robinson & Siebenmorgen (2000)
• Stellar population synthesis model of Bruzual & Charlot
• Radiative transfer that includes effect of small grains/PAHs (Siebenmorgen & Krugel)
• Simple model for the evolution of giant molecular clouds
5-9th September 2011 SED2011 conference
5-9th September 2011 SED2011 conference
5-9th September 2011 SED2011 conference
5-9th September 2011 SED2011 conference
5-9th September 2011 SED2011 conference
Fit to Arp220 with the Efstathiou et al model (Farrah et al 2003)
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00183-7111 – A young starburst?
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Mid-IR spectroscopy of AGN
• 8-13m spectrophotometry from the ground by Roche and collaborators
• Type 2 AGN showed moderate silicate absorption features
• Type 1 AGN featureless• Discovery of silicate emission features in the
Spitzer spectra of quasars by Siebenmorgen et al and Hao et al.
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Average spectra of Hao et al
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Tapered disc of Efstathiou & Rowan-Robinson (1995)
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Tapered disc model of NGC1068 (Galliano et al 2003)
Grid of tapered disc models
• Computed a grid of 36 tapered disc models
• Vary outer to inner disc radius in the range 20 to 100
• Vary equatorial 1000A optical depth in the range 750 to 1250
• Vary torus opening angle in the range 30-60degrees
• Compute spectra for 74 inclinations5-9th September 2011 SED2011 conference
Distribution of silicate strength of tapered disc models (blue) – AGN of
Spoon et al shown in red
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As previous slide but including all galaxies of Spoon et al with EW < 0.07
5-9th September 2011 SED2011 conference
Distribution of silicate strength of all tapered disc models + NLR dust with a
covering factor of 5%
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Fit to the Hao et al Seyfert 2 average with a tapered disc and NLR dust
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Phoenix
• A new code that calculates the ultraviolet to mm emission of galaxies
• Incorporates the stellar population synthesis model of Bruzual & Charlot
• Incorporates the starburst model of Efstathiou, Rowan-Robinson & Siebenmorgen
• Treats multiple scattering from grains
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Results from Phoenix
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Fit to the SED of a spiral galaxy
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Model of Efstathiou (2006)
• The model assumes four components
• A torus viewed edge-on• Dust at a temperature of
600K and a covering factor of 2%
• Dust at a temperature of 200K and a covering factor of 15%
• A highly obscured starburst
5-9th September 2011 SED2011 conference
New model of F10214 that fits Herschel data
• The model assumes an additional component of NLR dust at a temperature of 80K
• The covering factor of NLR dust is very high. It is very likely that we have stronger gravitational lensing of the NLR than the torus
5-9th September 2011 SED2011 conference
Conclusions
• We have a fairly good understanding of the infrared emission of starburst galaxies and AGN
• IRAS F10214+4724 is very special. Its unique spectrum is probably due to the gravitational lensing of the emission of NLR clouds.
5-9th September 2011 SED2011 conference