Edward Montiel - Publications

Affiliations: 
Louisiana State University, Baton Rouge, LA, United States 

5 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2020 Barr AG, Boogert A, DeWitt CN, Montiel E, Richter MJ, Lacy JH, Neufeld DA, Indriolo N, Pendleton Y, Chiar J, Tielens AGGM. High-resolution Infrared Spectroscopy of Hot Molecular Gas in AFGL 2591 and AFGL 2136: Accretion in the Inner Regions of Disks around Massive Young Stellar Objects The Astrophysical Journal. 900: 104. DOI: 10.3847/1538-4357/Abab05  0.487
2018 Dungee R, Boogert A, DeWitt CN, Montiel E, Richter MJ, Barr AG, Blake GA, Charnley SB, Indriolo N, Karska A, Neufeld DA, Smith RL, Tielens AGGM. High-resolution SOFIA/EXES Spectroscopy of SO Gas in the Massive Young Stellar Object MonR2 IRS3: Implications for the Sulfur Budget. The Astrophysical Journal. Letters. 868. PMID 30778373 DOI: 10.3847/2041-8213/Aaeda9  0.466
2014 Roman-Duval J, Gordon KD, Meixner M, Bot C, Bolatto A, Hughes A, Wong T, Babler B, Bernard JP, Clayton GC, Fukui Y, Galametz M, Galliano F, Glover S, Hony S, ... ... Montiel E, et al. Dust and gas in the magellanic clouds from the heritage herschel key project. II. Gas-to-dust ratio variations across interstellar medium phases Astrophysical Journal. 797. DOI: 10.1088/0004-637X/797/2/86  0.618
2013 Ballering NP, Rieke GH, Su KYL, Montiel E. A trend between cold debris disk temperature and stellar type: Implications for the formation and evolution of wide-orbit planets Astrophysical Journal. 775. DOI: 10.1088/0004-637X/775/1/55  0.531
2013 Clayton GC, Bond HE, Long LA, Meyer PI, Sugerman BEK, Montiel E, Sparks WB, Meakes MG, Chesneau O, De Marco O. Evolution of the 1919 ejecta of V605 aquilae Astrophysical Journal. 771. DOI: 10.1088/0004-637X/771/2/130  0.621
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