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Zhang, Lulu, Ho, Luis C. (2023) The Contribution of Evolved Stars to Polycyclic Aromatic Hydrocarbon Heating and Implications for Estimating Star Formation Rates. The Astrophysical Journal, 943 (1) 60 doi:10.3847/1538-4357/acab60

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Reference TypeJournal (article/letter/editorial)
TitleThe Contribution of Evolved Stars to Polycyclic Aromatic Hydrocarbon Heating and Implications for Estimating Star Formation Rates
JournalThe Astrophysical Journal
AuthorsZhang, LuluAuthor
Ho, Luis C.Author
Year2023 (January 1)Volume943
Issue1
PublisherAmerican Astronomical Society
DOIdoi:10.3847/1538-4357/acab60Search in ResearchGate
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Mindat Ref. ID15678093Long-form Identifiermindat:1:5:15678093:5
GUID0
Full ReferenceZhang, Lulu, Ho, Luis C. (2023) The Contribution of Evolved Stars to Polycyclic Aromatic Hydrocarbon Heating and Implications for Estimating Star Formation Rates. The Astrophysical Journal, 943 (1) 60 doi:10.3847/1538-4357/acab60
Plain TextZhang, Lulu, Ho, Luis C. (2023) The Contribution of Evolved Stars to Polycyclic Aromatic Hydrocarbon Heating and Implications for Estimating Star Formation Rates. The Astrophysical Journal, 943 (1) 60 doi:10.3847/1538-4357/acab60
In(2023, January) The Astrophysical Journal Vol. 943 (1) American Astronomical Society

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Zhang, Lulu, Ho, Luis C. (2023) Estimating Molecular Gas Content in Galaxies from Polycyclic Aromatic Hydrocarbon Emission. The Astrophysical Journal, 943 (1) 1 doi:10.3847/1538-4357/aca8f1
Xie, Yanxia, Ho, Luis C. (2019) A New Calibration of Star Formation Rate in Galaxies Based on Polycyclic Aromatic Hydrocarbon Emission. The Astrophysical Journal, 884 (2). 136pp. doi:10.3847/1538-4357/ab4200
Xie, Yanxia, Ho, Luis C., Li, Aigen, Shangguan, Jinyi (2018) A New Technique for Measuring Polycyclic Aromatic Hydrocarbon Emission in Different Environments. The Astrophysical Journal, 860 (2). 154pp. doi:10.3847/1538-4357/aac3dc
Xie, Yanxia, Ho, Luis C. (2022) The Ionization and Destruction of Polycyclic Aromatic Hydrocarbons in Powerful Quasars. The Astrophysical Journal, 925 (2) 218pp. doi:10.3847/1538-4357/ac32e2
Li, Yang A., Ho, Luis C., Shangguan, Jinyi (2023) The Subtle Effects of Mergers on Star Formation in Nearby Galaxies. The Astrophysical Journal, 953 (1) 91 doi:10.3847/1538-4357/acdddb
Zhuang, Ming-Yang, Ho, Luis C., Shangguan, Jinyi (2019) A New Method to Measure Star Formation Rates in Active Galaxies Using Mid-infrared Neon Emission Lines. The Astrophysical Journal, 873 (2). 103pp. doi:10.3847/1538-4357/ab0650
Yu, Niankun, Ho, Luis C., Wang, Jing (2022) Centrally Concentrated H i Distribution Enhances Star Formation in Galaxies. The Astrophysical Journal, 930 (1) 85 doi:10.3847/1538-4357/ac5f07
Yesuf, Hassen M., Ho, Luis C., Faber, S. M. (2021) What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82. The Astrophysical Journal, 923 (2) 205pp. doi:10.3847/1538-4357/ac27a7
Zhuang, Ming-Yang, Ho, Luis C., Shangguan, Jinyi (2019) Erratum: “A New Method to Measure Star Formation Rates in Active Galaxies Using Mid-infrared Neon Emission Lines” (2019, ApJ, 873, 103). The Astrophysical Journal, 875 (1). 78pp. doi:10.3847/1538-4357/ab126c
Yesuf, Hassen M., Ho, Luis C. (2020) Gas Content Regulates the Life Cycle of Star Formation and Black Hole Accretion in Galaxies. The Astrophysical Journal, 901 (1) 42pp. doi:10.3847/1538-4357/aba961
Yu, Si-Yue, Ho, Luis C., Wang, Jing (2021) Spiral Structure Boosts Star Formation in Disk Galaxies. The Astrophysical Journal, 917 (2) 88pp. doi:10.3847/1538-4357/ac0c77
 
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