activity
19982005
most citedThe Excitation of Extended Red Emission: New Constraints on its Carrier From HST Observations of NGC 7023

99 citations · 341 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph2005★ 99 cited

The Excitation of Extended Red Emission: New Constraints on its Carrier From HST Observations of NGC 7023

Adolf N. Witt, Karl D. Gordon, Uma P. Vijh +3

The carrier of the dust-associated photoluminescence process causing the extended red emission (ERE) in many dusty interstellar environments remains unidentified. Several competing…

astro-ph2003★ 39 cited

SMC-Type Interstellar Dust in the Milky Way

Lynne A. Valencic, Geoffrey C. Clayton, Karl Gordon +1

It is well known that the sightline toward HD 204827 in the cluster Trumpler 37 shows an UV extinction curve that does not follow CCM. However, when a dust component, foreground to…

astro-ph2003★ 79 cited

The Role of Polycyclic Aromatic Hydrocarbons in Ultraviolet Extinction. I. Probing small molecular PAHs

Geoffrey C. Clayton, Karl D. Gordon, Adolf N. Witt +7

We have obtained new STIS/HST spectra to search for structure in the ultraviolet interstellar extinction curve, with particular emphasis on a search for absorption features produce…

astro-ph2002

A New Feature in the Interstellar Extinction Curve at 2700 A: Diamonds in the Rough?

Geoffrey C. Clayton, Karl D. Gordon, Adolf N. Witt +7

Space Telescope Imaging Spectrograph (STIS) and archival International Ultraviolet Explorer (IUE) data were used to search for structure in the ultraviolet interstellar extinction…

astro-ph2001★ 59 cited

The Photophysics of the Carrier of Extended Red Emission

Tracy L. Smith, Adolf N. Witt

Interstellar dust contains a component which reveals its presence by emitting a broad, unstructured band of light in the 540 to 950 nm wavelength range, referred to as Extended Red…

astro-ph2000★ 34 cited

Dust Emission Features in NGC 7023 between 0.35 and 2.5 micron: Extended Red Emission (0.7 micron) and Two New Emission Features (1.15 and 1.5 micron)

K. D. Gordon, A. N. Witt, R. J. Rudy +6

We present 0.35 to 2.5 micron spectra of the south and northwest filaments in the reflection nebula NGC 7023. These spectra were used to test the theory of Seahra & Duley that carb…