The compact nucleus of the deep silicate absorption galaxy NGC 4418

A. S. Evans, E. E. Becklin, N. Z. Scoville, G. Neugebauer, B. T. Soifer, K. Matthews, M. Ressler, M. Werner, Marcia J Rieke

Research output: Contribution to journalArticle

35 Citations (Scopus)

Abstract

High-resolution Hubble Space Telescope (HST) near-infrared and Keck mid-infrared images of the heavily extinguished infrared-luminous galaxy NGC 4418 are presented. These data make it possible to observe the imbedded near-infrared structure on scales of 10-20 pc and to constrain the size of the mid-infrared-emitting region. The 1.1-2.2 μm data of NGC 4418 show no clear evidence of nuclear star clusters or of a reddened active galactic nucleus. Instead, the nucleus of the galaxy consists of a ∼100-200 pc linear structure with fainter structures extending radially outward. The near-infrared colors of the linear feature are consistent with a 10-300 Myr starburst suffering moderate levels (a few magnitudes) of visual extinction. At 7.9-24.5 μm NGC 4418 has estimated size upper limits in the range of 30-80 pc. These dimensions are consistent with the highest-resolution radio observations obtained to date of NGC 4418, as well as the size of 50-70 pc expected for a blackbody with a temperature derived from the 25, 60, and 100 μm flux densities of the galaxy. Further, a spectral energy distribution constructed from the multiwavelength mid-infrared observations shows the strong silicate absorption feature at 10 μm, consistent with previous mid-infrared observations of NGC 4418. An infrared surface brightness of ∼2.1 × 1013 L kpc-2 is derived for NGC 4418. Such a value, though consistent with the surface brightness of warm ultraluminous infrared galaxies [LIR (8-1000 μm) ≥ 10 12 L], such as IRAS 05189-2524 and IRAS 08572+3915, is not large enough to distinguish NGC 4418 as a galaxy powered by an active galactic nucleus, as opposed to a lower surface brightness starburst.

Original languageEnglish (US)
Pages (from-to)2341-2347
Number of pages7
JournalAstronomical Journal
Volume125
Issue number5 1769
DOIs
StatePublished - May 2003

Fingerprint

silicates
near infrared
silicate
galaxies
nuclei
brightness
Infrared Astronomy Satellite
active galactic nuclei
extinction
radio observation
radio
high resolution
star clusters
spectral energy distribution
Hubble Space Telescope
flux density
energy
color
temperature
distribution

Keywords

  • Galaxies: active
  • Galaxies: individual (NGC 4418)

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Evans, A. S., Becklin, E. E., Scoville, N. Z., Neugebauer, G., Soifer, B. T., Matthews, K., ... Rieke, M. J. (2003). The compact nucleus of the deep silicate absorption galaxy NGC 4418. Astronomical Journal, 125(5 1769), 2341-2347. https://doi.org/10.1086/374234

The compact nucleus of the deep silicate absorption galaxy NGC 4418. / Evans, A. S.; Becklin, E. E.; Scoville, N. Z.; Neugebauer, G.; Soifer, B. T.; Matthews, K.; Ressler, M.; Werner, M.; Rieke, Marcia J.

In: Astronomical Journal, Vol. 125, No. 5 1769, 05.2003, p. 2341-2347.

Research output: Contribution to journalArticle

Evans, AS, Becklin, EE, Scoville, NZ, Neugebauer, G, Soifer, BT, Matthews, K, Ressler, M, Werner, M & Rieke, MJ 2003, 'The compact nucleus of the deep silicate absorption galaxy NGC 4418', Astronomical Journal, vol. 125, no. 5 1769, pp. 2341-2347. https://doi.org/10.1086/374234
Evans AS, Becklin EE, Scoville NZ, Neugebauer G, Soifer BT, Matthews K et al. The compact nucleus of the deep silicate absorption galaxy NGC 4418. Astronomical Journal. 2003 May;125(5 1769):2341-2347. https://doi.org/10.1086/374234
Evans, A. S. ; Becklin, E. E. ; Scoville, N. Z. ; Neugebauer, G. ; Soifer, B. T. ; Matthews, K. ; Ressler, M. ; Werner, M. ; Rieke, Marcia J. / The compact nucleus of the deep silicate absorption galaxy NGC 4418. In: Astronomical Journal. 2003 ; Vol. 125, No. 5 1769. pp. 2341-2347.
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abstract = "High-resolution Hubble Space Telescope (HST) near-infrared and Keck mid-infrared images of the heavily extinguished infrared-luminous galaxy NGC 4418 are presented. These data make it possible to observe the imbedded near-infrared structure on scales of 10-20 pc and to constrain the size of the mid-infrared-emitting region. The 1.1-2.2 μm data of NGC 4418 show no clear evidence of nuclear star clusters or of a reddened active galactic nucleus. Instead, the nucleus of the galaxy consists of a ∼100-200 pc linear structure with fainter structures extending radially outward. The near-infrared colors of the linear feature are consistent with a 10-300 Myr starburst suffering moderate levels (a few magnitudes) of visual extinction. At 7.9-24.5 μm NGC 4418 has estimated size upper limits in the range of 30-80 pc. These dimensions are consistent with the highest-resolution radio observations obtained to date of NGC 4418, as well as the size of 50-70 pc expected for a blackbody with a temperature derived from the 25, 60, and 100 μm flux densities of the galaxy. Further, a spectral energy distribution constructed from the multiwavelength mid-infrared observations shows the strong silicate absorption feature at 10 μm, consistent with previous mid-infrared observations of NGC 4418. An infrared surface brightness of ∼2.1 × 1013 L⊙ kpc-2 is derived for NGC 4418. Such a value, though consistent with the surface brightness of warm ultraluminous infrared galaxies [LIR (8-1000 μm) ≥ 10 12 L⊙], such as IRAS 05189-2524 and IRAS 08572+3915, is not large enough to distinguish NGC 4418 as a galaxy powered by an active galactic nucleus, as opposed to a lower surface brightness starburst.",
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AU - Soifer, B. T.

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AU - Ressler, M.

AU - Werner, M.

AU - Rieke, Marcia J

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AB - High-resolution Hubble Space Telescope (HST) near-infrared and Keck mid-infrared images of the heavily extinguished infrared-luminous galaxy NGC 4418 are presented. These data make it possible to observe the imbedded near-infrared structure on scales of 10-20 pc and to constrain the size of the mid-infrared-emitting region. The 1.1-2.2 μm data of NGC 4418 show no clear evidence of nuclear star clusters or of a reddened active galactic nucleus. Instead, the nucleus of the galaxy consists of a ∼100-200 pc linear structure with fainter structures extending radially outward. The near-infrared colors of the linear feature are consistent with a 10-300 Myr starburst suffering moderate levels (a few magnitudes) of visual extinction. At 7.9-24.5 μm NGC 4418 has estimated size upper limits in the range of 30-80 pc. These dimensions are consistent with the highest-resolution radio observations obtained to date of NGC 4418, as well as the size of 50-70 pc expected for a blackbody with a temperature derived from the 25, 60, and 100 μm flux densities of the galaxy. Further, a spectral energy distribution constructed from the multiwavelength mid-infrared observations shows the strong silicate absorption feature at 10 μm, consistent with previous mid-infrared observations of NGC 4418. An infrared surface brightness of ∼2.1 × 1013 L⊙ kpc-2 is derived for NGC 4418. Such a value, though consistent with the surface brightness of warm ultraluminous infrared galaxies [LIR (8-1000 μm) ≥ 10 12 L⊙], such as IRAS 05189-2524 and IRAS 08572+3915, is not large enough to distinguish NGC 4418 as a galaxy powered by an active galactic nucleus, as opposed to a lower surface brightness starburst.

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