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Abstract:

Massive Population II galaxies undergoing the first phase of vigorous star formation after the initial Population III stage should have high energy densities and silicate-rich interstellar dust. We have modeled the resulting far-infrared spectral energy distributions (SEDs), demonstrating that they are shifted substantially to bluer ("warmer") wavelengths relative to the best fitting ones at z ≈ 3, and with strong outputs in the 10-40 μm range. When combined with a low level of emission by carbon dust, their SEDs match that of Haro 11, a local moderately low-metallicity galaxy undergoing a very young and vigorous starburst that is likely to approximate the relevant conditions in young Population II galaxies. We expect to see similar SEDs at high redshifts (z 5) given the youth of galaxies at this epoch. In fact, we find a progression with redshift in observed galaxy SEDs, from those resembling local ones at 2 ≲ z < 4 to a closer resemblance with Haro 11 at 5 ≲ z < 7. In addition to the insight on conditions in high-redshift galaxies, this result implies that estimates of the total infrared luminosities at z ∼ 6 based on measurements near λ ∼ 1 mm can vary by factors of 2-4, depending on the SED template used. Currently popular modified blackbodies or local templates can result in significant underestimates compared with the preferred template based on the SED of Haro 11. © 2018. The American Astronomical Society. All rights reserved.

Registro:

Documento: Artículo
Título:The Far-infrared Emission of the First Massive Galaxies
Autor:De Rossi, M.E.; Rieke, G.H.; Shivaei, I.; Bromm, V.; Lyu, J.
Filiación:Universidad de Buenos Aires, Facultad de Ciencias Exactas y Naturales y Ciclo Básico Común, Buenos Aires, Argentina
CONICET-Universidad de Buenos Aires, Instituto de Astronomía y Física Del Espacio (IAFE), Buenos Aires, Argentina
Steward Observatory, Department of Astronomy, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States
Department of Astronomy, University of Texas, 2515 Speedway, Austin, TX 78712-1205, United States
Palabras clave:galaxies: abundances; galaxies: evolution; galaxies: high-redshift; infrared: galaxies
Año:2018
Volumen:869
Número:1
DOI: http://dx.doi.org/10.3847/1538-4357/aaebf8
Título revista:Astrophysical Journal
Título revista abreviado:Astrophys. J.
ISSN:0004637X
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v869_n1_p_DeRossi

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Citas:

---------- APA ----------
De Rossi, M.E., Rieke, G.H., Shivaei, I., Bromm, V. & Lyu, J. (2018) . The Far-infrared Emission of the First Massive Galaxies. Astrophysical Journal, 869(1).
http://dx.doi.org/10.3847/1538-4357/aaebf8
---------- CHICAGO ----------
De Rossi, M.E., Rieke, G.H., Shivaei, I., Bromm, V., Lyu, J. "The Far-infrared Emission of the First Massive Galaxies" . Astrophysical Journal 869, no. 1 (2018).
http://dx.doi.org/10.3847/1538-4357/aaebf8
---------- MLA ----------
De Rossi, M.E., Rieke, G.H., Shivaei, I., Bromm, V., Lyu, J. "The Far-infrared Emission of the First Massive Galaxies" . Astrophysical Journal, vol. 869, no. 1, 2018.
http://dx.doi.org/10.3847/1538-4357/aaebf8
---------- VANCOUVER ----------
De Rossi, M.E., Rieke, G.H., Shivaei, I., Bromm, V., Lyu, J. The Far-infrared Emission of the First Massive Galaxies. Astrophys. J. 2018;869(1).
http://dx.doi.org/10.3847/1538-4357/aaebf8