ISO mid-infrared observations of normal star-forming galaxies: The key project sample

Daniel A. Dale, Nancy A. Silbermann, George Helou, Emmanuel Valjavec, Sangeeta Malhotra, Charles A. Beichman, James Brauher, Alessandra Contursi, Harriet L. Dinerstein, David J. Hollenbach, Deidre A. Hunter, Sonali Kolhatkar, Kwok Yung Lo, Steven D. Lord, Nanyao Y. Lu, Robert H. Rubin, Gordon J. Stacey, Harley A. Thronson, Michael W. Werner, Harold G. Corwin

Research output: Contribution to journalArticle

75 Citations (Scopus)

Abstract

We present mid-infrared maps and preliminary analysis for 61 galaxies observed with the ISOCAM instrument aboard the Infrared Space Observatory. Many of the general features of galaxies observed at optical wavelengths - spiral arms, disks, rings, and bright knots of emission - are also seen in the mid-infrared, except the prominent optical bulges are absent at 6.75 and 15 μm. In addition, the maps are quite similar at 6.75 and 15 μm, except for a few cases where a central starburst leads to lower Iv(6.75 μm)/Iv(15 μm) ratios in the inner region. We also present infrared flux densities and mid-infrared sizes for these galaxies. The mid-infrared color Iv(6.75 μm)/Iv(15 μm) shows a distinct trend with the far-infrared color Iv(60 μm)/Iv(100 μm). The quiescent galaxies in our sample [Iv(60 μm)/Iv(100 μm) ≲ 0.6] show Iv(6.75 μm)/Iv(15 μm) near unity, whereas this ratio drops significantly for galaxies with higher global heating intensity levels. Azimuthally averaged surface brightness profiles indicate the extent to which the mid-infrared flux is centrally concentrated, and provide information on the radial dependence of mid-infrared colors. The galaxies are mostly well resolved in these maps: almost half of them have <10% of their flux in the central resolution element. A comparison of optical and mid-infrared isophotal profiles indicates that the flux at 4400 Å near the optical outskirts of the galaxies is approximately 8 (7) times that at 6.75 μm (15 μm), comparable to observations of the diffuse quiescent regions of the Milky Way.

Original languageEnglish (US)
Pages (from-to)583-603
Number of pages21
JournalAstronomical Journal
Volume120
Issue number2
StatePublished - Aug 2000
Externally publishedYes

Fingerprint

galaxies
stars
color
observatory
heating
wavelength
Infrared Space Observatory (ISO)
profiles
project
unity
brightness
flux density
trends
rings
wavelengths
analysis
comparison
trend

Keywords

  • Galaxies: general
  • Galaxies: ISM

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Dale, D. A., Silbermann, N. A., Helou, G., Valjavec, E., Malhotra, S., Beichman, C. A., ... Corwin, H. G. (2000). ISO mid-infrared observations of normal star-forming galaxies: The key project sample. Astronomical Journal, 120(2), 583-603.

ISO mid-infrared observations of normal star-forming galaxies : The key project sample. / Dale, Daniel A.; Silbermann, Nancy A.; Helou, George; Valjavec, Emmanuel; Malhotra, Sangeeta; Beichman, Charles A.; Brauher, James; Contursi, Alessandra; Dinerstein, Harriet L.; Hollenbach, David J.; Hunter, Deidre A.; Kolhatkar, Sonali; Lo, Kwok Yung; Lord, Steven D.; Lu, Nanyao Y.; Rubin, Robert H.; Stacey, Gordon J.; Thronson, Harley A.; Werner, Michael W.; Corwin, Harold G.

In: Astronomical Journal, Vol. 120, No. 2, 08.2000, p. 583-603.

Research output: Contribution to journalArticle

Dale, DA, Silbermann, NA, Helou, G, Valjavec, E, Malhotra, S, Beichman, CA, Brauher, J, Contursi, A, Dinerstein, HL, Hollenbach, DJ, Hunter, DA, Kolhatkar, S, Lo, KY, Lord, SD, Lu, NY, Rubin, RH, Stacey, GJ, Thronson, HA, Werner, MW & Corwin, HG 2000, 'ISO mid-infrared observations of normal star-forming galaxies: The key project sample', Astronomical Journal, vol. 120, no. 2, pp. 583-603.
Dale DA, Silbermann NA, Helou G, Valjavec E, Malhotra S, Beichman CA et al. ISO mid-infrared observations of normal star-forming galaxies: The key project sample. Astronomical Journal. 2000 Aug;120(2):583-603.
Dale, Daniel A. ; Silbermann, Nancy A. ; Helou, George ; Valjavec, Emmanuel ; Malhotra, Sangeeta ; Beichman, Charles A. ; Brauher, James ; Contursi, Alessandra ; Dinerstein, Harriet L. ; Hollenbach, David J. ; Hunter, Deidre A. ; Kolhatkar, Sonali ; Lo, Kwok Yung ; Lord, Steven D. ; Lu, Nanyao Y. ; Rubin, Robert H. ; Stacey, Gordon J. ; Thronson, Harley A. ; Werner, Michael W. ; Corwin, Harold G. / ISO mid-infrared observations of normal star-forming galaxies : The key project sample. In: Astronomical Journal. 2000 ; Vol. 120, No. 2. pp. 583-603.
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abstract = "We present mid-infrared maps and preliminary analysis for 61 galaxies observed with the ISOCAM instrument aboard the Infrared Space Observatory. Many of the general features of galaxies observed at optical wavelengths - spiral arms, disks, rings, and bright knots of emission - are also seen in the mid-infrared, except the prominent optical bulges are absent at 6.75 and 15 μm. In addition, the maps are quite similar at 6.75 and 15 μm, except for a few cases where a central starburst leads to lower Iv(6.75 μm)/Iv(15 μm) ratios in the inner region. We also present infrared flux densities and mid-infrared sizes for these galaxies. The mid-infrared color Iv(6.75 μm)/Iv(15 μm) shows a distinct trend with the far-infrared color Iv(60 μm)/Iv(100 μm). The quiescent galaxies in our sample [Iv(60 μm)/Iv(100 μm) ≲ 0.6] show Iv(6.75 μm)/Iv(15 μm) near unity, whereas this ratio drops significantly for galaxies with higher global heating intensity levels. Azimuthally averaged surface brightness profiles indicate the extent to which the mid-infrared flux is centrally concentrated, and provide information on the radial dependence of mid-infrared colors. The galaxies are mostly well resolved in these maps: almost half of them have <10{\%} of their flux in the central resolution element. A comparison of optical and mid-infrared isophotal profiles indicates that the flux at 4400 {\AA} near the optical outskirts of the galaxies is approximately 8 (7) times that at 6.75 μm (15 μm), comparable to observations of the diffuse quiescent regions of the Milky Way.",
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AU - Dale, Daniel A.

AU - Silbermann, Nancy A.

AU - Helou, George

AU - Valjavec, Emmanuel

AU - Malhotra, Sangeeta

AU - Beichman, Charles A.

AU - Brauher, James

AU - Contursi, Alessandra

AU - Dinerstein, Harriet L.

AU - Hollenbach, David J.

AU - Hunter, Deidre A.

AU - Kolhatkar, Sonali

AU - Lo, Kwok Yung

AU - Lord, Steven D.

AU - Lu, Nanyao Y.

AU - Rubin, Robert H.

AU - Stacey, Gordon J.

AU - Thronson, Harley A.

AU - Werner, Michael W.

AU - Corwin, Harold G.

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N2 - We present mid-infrared maps and preliminary analysis for 61 galaxies observed with the ISOCAM instrument aboard the Infrared Space Observatory. Many of the general features of galaxies observed at optical wavelengths - spiral arms, disks, rings, and bright knots of emission - are also seen in the mid-infrared, except the prominent optical bulges are absent at 6.75 and 15 μm. In addition, the maps are quite similar at 6.75 and 15 μm, except for a few cases where a central starburst leads to lower Iv(6.75 μm)/Iv(15 μm) ratios in the inner region. We also present infrared flux densities and mid-infrared sizes for these galaxies. The mid-infrared color Iv(6.75 μm)/Iv(15 μm) shows a distinct trend with the far-infrared color Iv(60 μm)/Iv(100 μm). The quiescent galaxies in our sample [Iv(60 μm)/Iv(100 μm) ≲ 0.6] show Iv(6.75 μm)/Iv(15 μm) near unity, whereas this ratio drops significantly for galaxies with higher global heating intensity levels. Azimuthally averaged surface brightness profiles indicate the extent to which the mid-infrared flux is centrally concentrated, and provide information on the radial dependence of mid-infrared colors. The galaxies are mostly well resolved in these maps: almost half of them have <10% of their flux in the central resolution element. A comparison of optical and mid-infrared isophotal profiles indicates that the flux at 4400 Å near the optical outskirts of the galaxies is approximately 8 (7) times that at 6.75 μm (15 μm), comparable to observations of the diffuse quiescent regions of the Milky Way.

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