Yanling Wu, Ph.D.
Affiliations: | 2009 | Cornell University, Ithaca, NY, United States |
Website:
https://www.linkedin.com/in/yanling-wu-5110a232/Google:
"Yanling Wu"Mean distance: 16.44
Cross-listing: Astronomy Tree
Parents
Sign in to add mentor| Vassilis Charmandaris | grad student | 2009 | Cornell | |
| James Richard Houck | grad student | 2009 | Cornell | |
| (A mid-infrared study of Blue Compact Dwarf Galaxies.) | ||||
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Publications
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| Lira P, Videla L, Wu Y, et al. (2013) Modeling the nuclear infrared spectral energy distribution of type II active galactic nuclei Astrophysical Journal. 764 |
| Griffith RL, Tsai CW, Stern D, et al. (2011) Wise discovery of low-metallicity blue compact dwarf galaxies Astrophysical Journal Letters. 736 |
| Wu Y, Shi Y, Helou G, et al. (2011) THE MID-INFRARED LUMINOSITY FUNCTION AT z < 0.3 FROM 5MUSES: UNDERSTANDING THE STAR FORMATION/ACTIVE GALACTIC NUCLEUS BALANCE FROM A SPECTROSCOPIC VIEW The Astrophysical Journal. 734: 40 |
| Shi Y, Helou G, Yan L, et al. (2011) Extended Schmidt Law: Role Of Existing Stars In Current Star Formation The Astrophysical Journal. 733: 87 |
| Wu Y, Helou G, Armus L, et al. (2010) Infrared luminosities and aromatic features in the 24μm flux-limited sample of 5muses Astrophysical Journal. 723: 895-914 |
| Stacey GJ, Charmandaris V, Boulanger F, et al. (2010) The energetics of molecular gas in NGC 891 from H |
| Bernard-Salas J, Spoon HWW, Charmandaris V, et al. (2009) A spitzer high-resolution mid-infrared spectral atlas of starburst galaxies Astrophysical Journal, Supplement Series. 184: 230-247 |
| Wu Y, Charmandaris V, Huang J, et al. (2009) SPITZER/IRS 5-35 μm LOW-RESOLUTION SPECTROSCOPY OF THE 12 μm SEYFERT SAMPLE The Astrophysical Journal. 701: 658-676 |
| Lebouteiller V, Bernard-Salas J, Brandl B, et al. (2008) Chemical composition and mixing in giant H II regions: NGC 3603, 30 Doradus, and N66 Astrophysical Journal. 680: 398-419 |
| Wu Y, Charmandaris V, Houck JR, et al. (2008) Blue compact dwarf galaxies with Spitzer: The infrared/radio properties Astrophysical Journal. 676: 970-977 |