Ghent University Academic Bibliography

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Your filters: cql: author="Roman-Duval, Julia" or (type any "bookEditor issueEditor" and editor="Roman-Duval, Julia")

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Evidence of Dust Grain Evolution from Extinction Mapping in the IC 63 Photodissociation Region

Dries Van De Putte (UGent) , Karl Gordon (UGent) , Julia Roman-Duval, Benjamin F. Williams, Maarten Baes (UGent) , Kirill Tchernyshyov, Brandon L. Lawton and Heddy Arab

(2020) The Astrophysical Journal. 888.
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The influence of supernova remnants on the interstellar medium in the large Magellanic cloud seen at 20-600 µm wavelengths

Maša Lakićević, Jacco Th van Loon, Margaret Meixner, Karl Gordon (UGent) , Caroline Bot, Julia Roman-Duval, Brian Babler, Alberto Bolatto, Chad Engelbracht, Miroslav Filipović, et al.

(2015) ASTROPHYSICAL JOURNAL. 799(1).
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Dust and gas in the Magellanic clouds from the Heritage Herschel key project, II: gas-to-dust ratio variations across interstellar medium phases

Julia Roman-Duval, Karl Gordon (UGent) , Margaret Meixner, Caroline Bot, Alberto Bolatto, Annie Hughes, Tony Wong, Brian Babler, Jean-Philippe Bernard, Geoffrey C Clayton, et al.

(2014) ASTROPHYSICAL JOURNAL. 797(2).
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Dust and gas in the Magellanic clouds from the Heritage Herschel key project, I: dust properties and insights into the origin of the submillimeter excess emission

Karl Gordon (UGent) , Julia Roman-Duval, Caroline Bot, Margaret Meixner, Brian Babler, Jean-Philippe Bernard, Alberto Bolatto, Martha L Boyer, Geoffrey C Clayton, Charles Engelbracht, et al.

(2014) ASTROPHYSICAL JOURNAL. 797(2).

Academic Bibliography

Evidence of Dust Grain Evolution from Extinction Mapping in the IC 63 Photodissociation Region

The influence of supernova remnants on the interstellar medium in the large Magellanic cloud seen at 20-600 µm wavelengths

Dust and gas in the Magellanic clouds from the Heritage Herschel key project, II: gas-to-dust ratio variations across interstellar medium phases

Dust and gas in the Magellanic clouds from the Heritage Herschel key project, I: dust properties and insights into the origin of the submillimeter excess emission

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