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The Effect of Dust Geometry on the Lyα Output of Galaxies

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The Effect of Dust Geometry on the Lyα Output of Galaxies
Id. 49267259
Titulo The Effect of Dust Geometry on the Lyα Output of Galaxies
Autor(es) Scarlata, C.
Colbert, J.
Teplitz, H. I.
Panagia, N.
Hayes, M.
Siana, B.
Rau, A.
Francis, P.
Caon, A.
Pizzella, A.
Bridge, C.
Localización http://authors.library.caltech.edu/16578/1/Scarlata2009p6235Astrophys_J_Lett.pdf
Scarlata, C. and Colbert, J. and Teplitz, H. I. and Panagia, N. and Hayes, M. and Siana, B. and Rau, A. and Francis, P. and Caon, A. and Pizzella, A. and Bridge, C. (2009) The Effect of Dust Geometry on the Lyα Output of Galaxies. Astrophysical Journal Letters, 704 (2). L98-L102. ISSN 0004-637X http://resolver.caltech.edu/CaltechAUTHORS:20091104-113041493
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Descripción We present the optical spectroscopic follow-up of 31 z = 0.3 Lyα emitters, previously identified by Deharveng et al. We find that 17% of the Lyα emitters have line ratios that require the hard ionizing continuum produced by an active galactic nucleus. The uniform dust screen geometry traditionally used in studies similar to ours is not able to simultaneously reproduce the observed high Lyα/Hα and Hα/Hβ line ratios. We consider different possibilities for the geometry of the dust around the emitting sources. We find that also a uniform mixture of sources and dust does not reproduce the observed line ratios. Instead, these are well reproduced by a clumpy dust screen. This more realistic treatment of the geometry results in extinction corrected (Lyα/Hα) C values consistent with case B recombination theory, whereas a uniform dust screen model would imply values (Lyα/Hα) C higher than 8.7. Our analysis shows that there is no need to invoke ad hoc multiphase media in which the Lyα photons only scatter between the dusty clouds and eventually escape
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Estructura Atomic
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Relación [References] http://resolver.caltech.edu/CaltechAUTHORS:20091104-113041493
[References] http://authors.library.caltech.edu/16578/
Fecha de contribución 05-nov-2009
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