The extreme star formation activity of Aarp 299 revealed by spitzer IRS spectral mapping

Almudena Alonso-Herrero, George H. Rieke, Luis Colina, Miguel Pereira-Santaella, MacArena García-Marín, J. D.T. Smith, Bernhard Brandl, Vassilis Charmandaris, Lee Armus

Research output: Contribution to journalArticle

33 Scopus citations

Abstract

We present Spitzer/IRS spectral mapping observations of the luminous infrared galaxy Arp 299 (IC 694 + NGC 3690) covering the central 45″ 9 kpc. The integrated mid-IR spectrum of Arp 299 is similar to that of local starbursts despite its strongly interacting nature and high-IR luminosity, L IR 6 × 1011 L . This is explained because the star formation (probed by, e.g., high [Ne III]15.56 μm/[Ne II]12.81 μm line ratios) is spread across at least 6-8kpc. Moreover, a large fraction of this star formation is taking place in young regions of moderate mid-IR optical depths such as the C+C′ complex in the overlap region between the two galaxies and in H II regions in the disks of the galaxies. It is only source A, the nuclear region of IC 694, which shows the typical mid-IR characteristics of ultraluminous infrared galaxies (ULIRGs; L IR > 1012 L ), that is, very compact (less than 1kpc) and dust-enshrouded star formation resulting in a deep silicate feature and moderate equivalent widths of the polycyclic aromatic hydrocarbons. The nuclear region of NGC 3690, known as source B1, hosts a low-luminosity active galactic nucleus (AGN) and is surrounded by regions of star formation. Although the high-excitation [Ne V]14.32 μm line typical of AGN is not detected in B1, its upper limit is consistent with the value expected from the X-ray luminosity. The AGN emission is detected in the form of a strong hot-dust component that accounts for 80%-90% of the 6 μm luminosity of B1. The similarity between the Arp 299 integrated mid-IR spectrum and those of high-z ULIRGs suggests that Arp 299 may represent a local example, albeit with lower IR luminosity and possibly higher metallicity, of the star formation processes occurring at high-z.

Original languageEnglish (US)
Pages (from-to)660-675
Number of pages16
JournalAstrophysical Journal
Volume697
Issue number1
DOIs
StatePublished - Jan 1 2009

    Fingerprint

Keywords

  • Galaxies: Seyfert
  • Galaxies: evolution
  • Galaxies: individual (Arp299)
  • Galaxies: nuclei
  • Galaxies: structure
  • Infrared: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Alonso-Herrero, A., Rieke, G. H., Colina, L., Pereira-Santaella, M., García-Marín, M., Smith, J. D. T., Brandl, B., Charmandaris, V., & Armus, L. (2009). The extreme star formation activity of Aarp 299 revealed by spitzer IRS spectral mapping. Astrophysical Journal, 697(1), 660-675. https://doi.org/10.1088/0004-637X/697/1/660