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The Spectrum of the Planetary Nebula NGC 6884
DOI: 10.1086/312969 Bibcode: 1997ApJS..108..503H

Feibelman, Walter A.; Hyung, Siek; Aller, Lawrence H.

The bright, compact, moderately high-excitation planetary nebula, NGC 6884 (Perek-Kohoutek 82 +07°1) has a rich spectrum promising good diagnostics and offering a good target for the Hamilton Echelle Spectrograph at Lick Observatory. We combine International Ultraviolet Explorer (IUE), near-UV, visual, and IR data to obtain N(ion)/N(H+)…

1997 The Astrophysical Journal Supplement Series
IUE 19
Infrared Photometry of 487 Sources in the Inner Regions of NGC 5128 (Centaurus A)
DOI: 10.1086/312982 Bibcode: 1997ApJS..109..397A

Minniti, Dante; Alonso, M. Victoria

We study the sources present in the inner 3 kpc region of NGC 5128 (Cen A), most of which are star clusters of different ages. Photometry of archival Hubble Space Telescope WFPC images (F675W filter) is complemented with IR photometry (JHK' filters) obtained with the IRAC2B infrared array camera at the ESO/MPI 2.2 m telescope. From IR color maps w…

1997 The Astrophysical Journal Supplement Series
eHST 14
The IUE Spectrum of the ``O VI Sequence'' Planetary Nebula IC 2003
DOI: 10.1086/312984 Bibcode: 1997ApJS..109..481F

Feibelman, Walter A.

We present archival low- and high-dispersion, as well as new SWP high-dispersion, IUE data of the ``O VI sequence'' planetary nebula IC 2003 that has not been studied extensively in the UV. Contrary to earlier UV studies, IC 2003 shows a rich spectrum of stellar and nebular emission lines. Nearly 60 new emission line fluxes are presented for He II…

1997 The Astrophysical Journal Supplement Series
IUE 11
The Greatly Expanded IUE Spectrum of the Planetary Nebula NGC 2371-2 and Its Central Star
DOI: 10.1086/313033 Bibcode: 1997ApJS..112..193F

Feibelman, Walter A.

Early IUE low-dispersion SWP and LWR spectra have been reexamined by means of refined current data reduction routines. These spectra contain much more information than was reported in 1981. A high-dispersion SWP spectrum was obtained in 1994 from which more than 80 emission and absorption features were identified, and log Ne = 3.0 +/- 0…

1997 The Astrophysical Journal Supplement Series
IUE 8