Showing 1–20 of 23 results
/ Date/ Name
Feb 10, 2019The nitrogen carrier in protoplanetary disksJul 22, 2020High Resolution Infrared Spectroscopy of Hot Molecular Gas in AFGL 2591 and AFGL 2136: Accretion in the Inner Regions of Disks Around Massive Young Stellar ObjectsApr 4, 2004R=100,000 Spectroscopy of Photodissociation Regions: H2 Rotational Lines in the Orion BarApr 2, 2008[Ne II] Observations of Gas Motions in Compact and Ultracompact H II RegionsJun 10, 2017IRTF/TEXES Observations of the HII Regions H1 and H2 in the Galactic CentreJan 30, 2025High-precision measurements of electric-dipole-transition amplitudes in excited states of $^{208}$Pb using Faraday rotation spectroscopyAug 10, 2010NGC 4102: High Resolution Infrared Observations of a Nuclear Starburst RingFeb 20, 2013Interpretation of Infrared Vibration-Rotation Spectra of Interstellar and Circumstellar MoleculesAug 29, 2015Detection of water vapor in the terrestrial planet forming region of a transition diskMar 28, 2017H2, CO, and Dust Absorption through Cold Molecular CloudsOct 15, 2002Observations of [S IV] 10.5 micron and [Ne II] 12.8 micron in Two Halo Planetary Nebulae: Implications for Chemical Self-EnrichmentJun 27, 2020Vertically-resolved observations of Jupiter's quasi-quadrennial oscillation from 2012 to 2019Nov 30, 2020High-Resolution Mid-Infrared Spectroscopy of GV Tau N: Surface Accretion and Detection of Ammonia in a Young Protoplanetary DiskJul 9, 2018Spectrally Resolved Mid-Infrared Molecular Emission from Protoplanetary Disks and the Chemical Fingerprint of Planetesimal FormationApr 9, 2009High Resolution Spectroscopy of [NeII] Emission from AA Tau and GM AurMar 15, 2004H2 Mid-IR Pure Rotational Emission from Young Stars: The TEXES/IRTF SurveyJun 12, 2012Ionized Gas in the Galactic Center: New Observations and InterpretationAug 9, 2012A Comparative Astrochemical Study Of The High-Mass Protostellar Objects NGC 7538 IRS 9 and IRS 1Jun 6, 2005Mass Flows in Cometary UCHII RegionsJun 24, 2021The Transition from Diffuse Molecular Gas to Molecular Cloud Material in Taurus