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Title: THE ROLE OF STARBURST-ACTIVE GALACTIC NUCLEUS COMPOSITES IN LUMINOUS INFRARED GALAXY MERGERS: INSIGHTS FROM THE NEW OPTICAL CLASSIFICATION SCHEME

Abstract

We investigate the fraction of starbursts, starburst-active galactic nucleus (AGN) composites, Seyferts, and low-ionization narrow emission-line region galaxies (LINERs) as a function of infrared luminosity (L{sub IR}) and merger progress for approx500 infrared (IR)-selected galaxies. Using the new optical classifications afforded by the extremely large data set of the Sloan Digital Sky Survey, we find that the fraction of LINERs in IR-selected samples is rare (<5%) compared with other spectral types. The lack of strong IR emission in LINERs is consistent with recent optical studies suggesting that LINERs contain AGN with lower accretion rates than in Seyfert galaxies. Most previously classified IR-luminous LINERs are classified as starburst-AGN composite galaxies in the new scheme. Starburst-AGN composites appear to 'bridge' the spectral evolution from starburst to AGN in ULIRGs. The relative strength of the AGN versus starburst activity shows a significant increase at high IR luminosity. In ULIRGs (L{sub IR} > 10{sup 12} L{sub sun}), starburst-AGN composite galaxies dominate at early-intermediate stages of the merger, and AGN galaxies dominate during the final merger stages. Our results are consistent with models for IR-luminous galaxies where mergers of gas-rich spirals fuel both starburst and AGN, and where the AGN becomes increasingly dominant during themore » final merger stages of the most luminous IR objects.« less

Authors:
;
Publication Date:
OSTI Identifier:
21392291
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal
Additional Journal Information:
Journal Volume: 709; Journal Issue: 2; Other Information: DOI: 10.1088/0004-637X/709/2/884; Journal ID: ISSN 0004-637X
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; EMISSION; GALACTIC EVOLUTION; IONIZATION; LUMINOSITY; SEYFERT GALAXIES; EVOLUTION; GALAXIES; OPTICAL PROPERTIES; PHYSICAL PROPERTIES

Citation Formats

Yuan, T -T, Kewley, L J, and Sanders, D. B., E-mail: yuantt@ifa.hawaii.ed, E-mail: kewley@ifa.hawaii.ed, E-mail: sanders@ifa.hawaii.ed. THE ROLE OF STARBURST-ACTIVE GALACTIC NUCLEUS COMPOSITES IN LUMINOUS INFRARED GALAXY MERGERS: INSIGHTS FROM THE NEW OPTICAL CLASSIFICATION SCHEME. United States: N. p., 2010. Web. doi:10.1088/0004-637X/709/2/884.
Yuan, T -T, Kewley, L J, & Sanders, D. B., E-mail: yuantt@ifa.hawaii.ed, E-mail: kewley@ifa.hawaii.ed, E-mail: sanders@ifa.hawaii.ed. THE ROLE OF STARBURST-ACTIVE GALACTIC NUCLEUS COMPOSITES IN LUMINOUS INFRARED GALAXY MERGERS: INSIGHTS FROM THE NEW OPTICAL CLASSIFICATION SCHEME. United States. https://doi.org/10.1088/0004-637X/709/2/884
Yuan, T -T, Kewley, L J, and Sanders, D. B., E-mail: yuantt@ifa.hawaii.ed, E-mail: kewley@ifa.hawaii.ed, E-mail: sanders@ifa.hawaii.ed. 2010. "THE ROLE OF STARBURST-ACTIVE GALACTIC NUCLEUS COMPOSITES IN LUMINOUS INFRARED GALAXY MERGERS: INSIGHTS FROM THE NEW OPTICAL CLASSIFICATION SCHEME". United States. https://doi.org/10.1088/0004-637X/709/2/884.
@article{osti_21392291,
title = {THE ROLE OF STARBURST-ACTIVE GALACTIC NUCLEUS COMPOSITES IN LUMINOUS INFRARED GALAXY MERGERS: INSIGHTS FROM THE NEW OPTICAL CLASSIFICATION SCHEME},
author = {Yuan, T -T and Kewley, L J and Sanders, D. B., E-mail: yuantt@ifa.hawaii.ed, E-mail: kewley@ifa.hawaii.ed, E-mail: sanders@ifa.hawaii.ed},
abstractNote = {We investigate the fraction of starbursts, starburst-active galactic nucleus (AGN) composites, Seyferts, and low-ionization narrow emission-line region galaxies (LINERs) as a function of infrared luminosity (L{sub IR}) and merger progress for approx500 infrared (IR)-selected galaxies. Using the new optical classifications afforded by the extremely large data set of the Sloan Digital Sky Survey, we find that the fraction of LINERs in IR-selected samples is rare (<5%) compared with other spectral types. The lack of strong IR emission in LINERs is consistent with recent optical studies suggesting that LINERs contain AGN with lower accretion rates than in Seyfert galaxies. Most previously classified IR-luminous LINERs are classified as starburst-AGN composite galaxies in the new scheme. Starburst-AGN composites appear to 'bridge' the spectral evolution from starburst to AGN in ULIRGs. The relative strength of the AGN versus starburst activity shows a significant increase at high IR luminosity. In ULIRGs (L{sub IR} > 10{sup 12} L{sub sun}), starburst-AGN composite galaxies dominate at early-intermediate stages of the merger, and AGN galaxies dominate during the final merger stages. Our results are consistent with models for IR-luminous galaxies where mergers of gas-rich spirals fuel both starburst and AGN, and where the AGN becomes increasingly dominant during the final merger stages of the most luminous IR objects.},
doi = {10.1088/0004-637X/709/2/884},
url = {https://www.osti.gov/biblio/21392291}, journal = {Astrophysical Journal},
issn = {0004-637X},
number = 2,
volume = 709,
place = {United States},
year = {Mon Feb 01 00:00:00 EST 2010},
month = {Mon Feb 01 00:00:00 EST 2010}
}