Henrik Willem Walter Spoon
Affiliations: | 2003- | Cornell University, Ithaca, NY, United States |
Website:
http://spoon.astro.cornell.eduGoogle:
"Henrik Spoon"Mean distance: (not calculated yet)
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Publications
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| Gowardhan A, Spoon H, Riechers DA, et al. (2018) The Dual Role of Starbursts and Active Galactic Nuclei in Driving Extreme Molecular Outflows The Astrophysical Journal. 859: 35 |
| Stone M, Veilleux S, González-Alfonso E, et al. (2018) Constraints on the OH-to-H Abundance Ratio in Infrared-bright Galaxies Derived from the Strength of the OH 35μm Absorption Feature The Astrophysical Journal. 853: 132 |
| Petric AO, Armus L, Flagey N, et al. (2018) Warm Molecular Hydrogen in Nearby, Luminous Infrared Galaxies The Astronomical Journal. 156: 295 |
| Pearson C, Rigopoulou D, Hurley P, et al. (2016) HERUS: A CO Atlas from SPIRE Spectroscopy of Local ULIRGs Astrophysical Journal Supplement Series. 227: 9 |
| Brisbin D, Ferkinhoff C, Nikola T, et al. (2015) Strong C+ emission in galaxies at z ∼ 1-2: Evidence for cold flow accretion powered star formation in the early universe Astrophysical Journal. 799 |
| Sargsyan L, Samsonyan A, Lebouteiller V, et al. (2014) Star formation rates from [C II] 158 μm and mid-infrared emission lines for starbursts and active galactic nuclei Astrophysical Journal. 790 |
| Dicken D, Tadhunter C, Morganti R, et al. (2014) Spitzer MID-IR spectroscopy of powerful 2Jy and 3CRR radio galaxies. II : Agn power indicators and unification The Astrophysical Journal. 788: 98-119 |
| Inami H, Armus L, Charmandaris V, et al. (2013) Mid-infrared atomic fine-structure emission-line spectra of luminous infrared galaxies: Spitzer/IRS spectra of the goals sample Astrophysical Journal. 777 |
| Norris RP, Lenc E, Roy AL, et al. (2012) The radio core of the ultraluminous infrared galaxy F00183-7111: Watching the birth of a quasar Monthly Notices of the Royal Astronomical Society. 422: 1453-1459 |
| Urrutia T, Lacy M, Spoon H, et al. (2012) Spitzer observations of young red quasars Astrophysical Journal. 757 |