Extended Red Emission and the evolution of carbonaceous nanograins in NGC 7023
History of globulettes in the Milky Way
PDR Model Mapping of Physical Conditions via Spitzer/IRS Spectroscopy of H2: Theoretical Success toward NGC 2023-South
Photoluminescence by Interstellar Dust
Polycyclic aromatic hydrocarbon emission model in photodissociation regions - II. Application to the polycyclic aromatic hydrocarbon and fullerene emission in NGC 7023
Properties of Polycyclic Aromatic Hydrocarbons in the Northwest Photon Dominated Region of NGC 7023. III. Quantifying the Traditional Proxy for PAH Charge and Assessing its Role
Properties of Polycyclic Aromatic Hydrocarbons in the Northwest Photon Dominated Region of NGC 7023. II. Traditional PAH Analysis Using k-means as a Visualization Tool
Properties of Polycyclic Aromatic Hydrocarbons in the Northwest Photon Dominated Region of NGC 7023. I. PAH Size, Charge, Composition, and Structure Distribution
The 6.2 mm PAH Feature and the Role of Nitrogen: Revisited
The Charge State of Polycyclic Aromatic Hydrocarbons across a Reflection Nebula, an H II Region, and a Planetary Nebula
The Excitation of Extended Red Emission: New Constraints on Its Carrier from Hubble Space Telescope Observations of NGC 7023
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/HRC, ACS/WFC, NICMOS, NICMOS/NIC2
Temporal Coverage
2003-09-12T07:53:21Z/2004-01-25T17:46:35Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Gordon et al., 2005, 'The Exciting Wavelength of Extended Red Emission', 1.0, European Space Agency, https://doi.org/10.5270/esa-es6mymy