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Cited by 202

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Radial Variation of Attenuation and Star Formation in the Largest Late‐Type Disks Observed with GALEX

Open access
Boissier, Samuel, Gil de Paz, Armando, Boselli, Alessandro, Madore, Barry F., Buat, Veronique, Cortese, Luca, Burgarella, Denis, Mateos, Juan Carlos Munoz, Barlow, Tom A., Forster, Karl, Friedman, Peter G., Martin, D. Christopher, Morrissey, Patrick, Neff, Susan G., Schiminovich, David, Seibert, Mark, Small, Todd, Wyder, Ted K., Bianchi, Luciana, Donas, Jose, Heckman, Timothy M., Lee, Young‐Wook, Milliard, Bruno, Rich, R. Michael, Szalay, Alex S., Welsh, Barry Y., Yi, Sukyoung K.·2007·The Astrophysical Journal Supplement Series

Abstract

For a sample of 43 nearby, late-type galaxies, we have investigated the radial variation of both the current star formation rate and the dust-induced UV light attenuation. To do this we have cross-correlated IRAS images and GALEX observations for each of these galaxies and compiled observations of the gas (CO and H I) and metal-abundance gradients found in the literature. We find that attenuation correlates with metallicity. We then use the UV profiles, corrected for attenuation, to study several variants of the Schmidt law and conclude that our results are compatible with a simple law similar to the one of Kennicutt extending smoothly to lower surface densities, but with considerable scatter. We do not detect an abrupt break in the UV light at the threshold radius derived from Hα data (at which the Hα profile shows a break and beyond which only a few H II regions are usually found). We interpret the Hα sudden break not as a change in the star formation regime (as often suggested), but as the vanishingly small number of ionizing stars corresponding to low levels of star formation.

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Metadata

Authors
Boissier, S., Gil de Paz, A., Boselli, A., Madore, B. F., Buat, V., Cortese, L., Burgarella, D., Mateos, J. C. M., Barlow, T. A., Forster, K., Friedman, P. G., Martin, D. C., Morrissey, P., Neff, S. G., Schiminovich, D., Seibert, M., Small, T., Wyder, T. K., Bianchi, L., Donas, J., Heckman, T. M., Lee, Y., Milliard, B., Rich, R. M., Szalay, A. S., Welsh, B. Y., & Yi, S. K.
Venue
The Astrophysical Journal Supplement Series
Published
2007-12
Volume
173
Issue
2
Pages
524-537
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W2076489605
Cited by
202
References
2
FWCI
16.10
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Radial Variation of Attenuation and Star Formation in the Largest Late‐Type Disks Observed with GALEX. https://app.cochat.ai/papers/10.1086/516642
The paper
Boissier, S., Gil de Paz, A., Boselli, A., Madore, B. F., Buat, V., Cortese, L., Burgarella, D., Mateos, J. C. M., Barlow, T. A., Forster, K., Friedman, P. G., Martin, D. C., Morrissey, P., Neff, S. G., Schiminovich, D., Seibert, M., Small, T., Wyder, T. K., Bianchi, L., . . . Yi, S. K. (2007). Radial Variation of Attenuation and Star Formation in the Largest Late‐Type Disks Observed with GALEX. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/516642

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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