D
D. Riebel
Researcher at Johns Hopkins University
Publications - 25
Citations - 1328
D. Riebel is an academic researcher from Johns Hopkins University. The author has contributed to research in topics: Stars & Asymptotic giant branch. The author has an hindex of 15, co-authored 25 publications receiving 1265 citations. Previous affiliations of D. Riebel include United States Naval Academy.
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Journal ArticleDOI
The dust budget of the small magellanic cloud: are asymptotic giant branch stars the primary dust source at low metallicity?
Martha L. Boyer,Sundar Srinivasan,D. Riebel,Iain McDonald,J. Th. van Loon,Geoffrey C. Clayton,Karl D. Gordon,Margaret Meixner,B. A. Sargent,Greg Sloan +9 more
TL;DR: In this article, the authors estimate the total dust input from the cool evolved stars in the Small Magellanic Cloud, using the 8 μm excess emission as a proxy for the dust-production rate.
Journal ArticleDOI
HERschel Inventory of the Agents of Galaxy Evolution (HERITAGE): the Large Magellanic Cloud dust
Margaret Meixner,Margaret Meixner,Frédéric Galliano,Sacha Hony,Julia Roman-Duval,Thomas P. Robitaille,Pasquale Panuzzo,Marc Sauvage,Karl D. Gordon,Chad Engelbracht,Karl Misselt,Koryo Okumura,Tracy L. Beck,J.-P. Bernard,Alberto D. Bolatto,Caroline Bot,Martha L. Boyer,S. Bracker,Lynn Redding Carlson,Geoffrey C. Clayton,C.-H. R. Chen,Ed Churchwell,Yasuo Fukui,Maud Galametz,Joseph L. Hora,Annie Hughes,Remy Indebetouw,Frank P. Israel,Akiko Kawamura,Francisca Kemper,Sungeun Kim,E. Kwon,Brandon Lawton,Aigen Li,Knox S. Long,Massimo Marengo,S. C. Madden,Mikako Matsuura,Joana M. Oliveira,Toshikazu Onishi,Masaaki Otsuka,Deborah Paradis,Albrecht Poglitsch,D. Riebel,William T. Reach,William T. Reach,Monica Rubio,Benjamin A. Sargent,Marta Sewilo,Joshua D. Simon,Ramin A. Skibba,Linda J. Smith,Sundar Srinivasan,Alexander G. G. M. Tielens,J. Th. van Loon,Barbara A. Whitney,Paul M. Woods +56 more
TL;DR: In this paper, the authors used the Herschel Space Observatory's PACS and SPIRE photometry cameras to image a 2° × 8° strip through the Large and Small Magellanic Clouds (LMC and SMC) at a position angle of 22.5°.
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The SAGE-Spec Spitzer Legacy programme: the life-cycle of dust and gas in the Large Magellanic Cloud - Point source classification I
Paul M. Woods,Joana M. Oliveira,Francisca Kemper,J. Th. van Loon,Benjamin A. Sargent,Mikako Matsuura,Ryszard Szczerba,Kevin Volk,Albert A. Zijlstra,Greg Sloan,Eric Lagadec,Eric Lagadec,Iain McDonald,Olivia Jones,Varoujan Gorjian,Kathleen E. Kraemer,Clio Gielen,Margaret Meixner,Robert Blum,Marta Sewilo,D. Riebel,Bernie Shiao,C.-H. R. Chen,Martha L. Boyer,Remy Indebetouw,Remy Indebetouw,Vallia Antoniou,J.-P. Bernard,Marvin L. Cohen,C. Dijkstra,Maud Galametz,Frédéric Galliano,Karl D. Gordon,J. Harris,Sacha Hony,Joseph L. Hora,A. Kawamura,Brandon Lawton,Jarron Leisenring,S. C. Madden,Massimo Marengo,Massimo Marengo,C. McGuire,A. J. Mulia,B. O’Halloran,K. Olsen,R. Paladini,D. Paradis,William T. Reach,D. Rubin,Karin Sandstrom,Karin Sandstrom,Igor Soszyński,Angela Speck,Sundar Srinivasan,Sundar Srinivasan,Alexander G. G. M. Tielens,E. van Aarle,S. D. Van Dyk,H. Van Winckel,Uma P. Vijh,B. Whitney,A. N. Wilkins +62 more
TL;DR: In this article, a decision-tree method of object classification based on infrared spectral features, continuum and spectral energy distribution shape, bolometric luminosity, cluster membership and variability information was used to classify the SAGE-Spec sample of point sources.
Journal ArticleDOI
The mass-loss return from evolved stars to the large magellanic cloud. vi. luminosities and mass-loss rates on population scales
TL;DR: The Grid of Red Supergiant and Asymptotic Giant Branch ModelS (GRAMS) as discussed by the authors is a pre-computed grid of 80,843 radiative transfer models of evolved stars and circumstellar dust shells composed of either silicate or carbonaceous dust.
Journal ArticleDOI
The Dust Budget of the SMC: Are AGB Stars the Primary Dust Source at Low Metallicity?
Martha L. Boyer,Sundar Srinivasan,D. Riebel,Iain McDonald,J. Th. van Loon,Geoffrey C. Clayton,Karl D. Gordon,Margaret Meixner,B. A. Sargent,Gregory C. Sloan +9 more
TL;DR: In this article, the authors estimate the total dust input from the cool evolved stars in the Small Magellanic Cloud (SMC), using the 8 micron excess emission as a proxy for the dust-production rate.