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Nanyao Y. Lu
Researcher at California Institute of Technology
Publications - 90
Citations - 10692
Nanyao Y. Lu is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 44, co-authored 90 publications receiving 10248 citations. Previous affiliations of Nanyao Y. Lu include Jet Propulsion Laboratory.
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IRAS galaxies at low galactic and high supergalactic latitudes
TL;DR: Based on IR colors, 371 IRAS point sources with absolute value of b = 2-16 deg (b = galactic latitude) were selected for study at H I 21 cm as potential galaxies: 25 percent (93) of these sources are galaxies with redshifts less than 8000 km/s based on H I spectra as mentioned in this paper.
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The Mid-Infrared Spectra of Normal Galaxies
TL;DR: The mid-infrared spectra obtained by ISO-PHOT reveal the interstellar medium emission from galaxies powered by star formation to be strongly dominated by the aromatic features at 6.2, 7.7, 8.6 and 11.3 mu.
Journal Article
Mid-infrared observations of NGC 6946 with ISOCAM.
Sangeeta Malhotra,George Helou,C. A. Beichman,S. D. Lord,Nanyao Y. Lu,David Hollenbach,Robert H. Rubin,Harley A. Thronson,G. Stasey,Harriet L. Dinerstein,Michael Werner,Deidre A. Hunter,K. Y. Lo +12 more
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Disk Galaxies in the Outer Local Supercluster: Optical CCD Surface Photometry and Distribution of Galaxy Disk Parameters
TL;DR: Lu et al. as mentioned in this paper used B-band CCD surface photometry on a sample of 76 disk galaxies brighter than B_T = 14.5 mag in the Uppsala General Catalogue of Galaxies, which are confined within a volume located in the outer part of the Local Supercluster.
Posted Content
ISOCAM Observations of NGC 6946: Mid-IR Structure
Sangeeta Malhotra,George Helou,D. Van Buren,M. Kong,Chas Beichman,Harriet L. Dinerstein,David J. Hollenbach,Deidre A. Hunter,K. Y. Lo,S. D. Lord,Nanyao Y. Lu,Robert H. Rubin,Gordon J. Stacey,Harley A. Thronson,Michael W. Werner +14 more
TL;DR: In this paper, a spiral galaxy NGC 6946 was observed with ISO-CAM in the mid-infrared, achieving 7 arcsec resolution and sub-MJy/steradian sensitivity.