Aims. We present line identifications in the 1700 to 10 400 Å region for the Weigelt blobs B
and D, located 0 ″. 1 to 0 ″. 3 NNW of Eta Carinae. The aim of this work is to characterize …

Measured wave-lengths and intensities of 143 emission lines between 6666 and 9122A in
the spectrum of Eta Carinae are presented, based on four Radcliffe coudé spectra. 28 well …

We present numerical simulations that reproduce the salient features of the amazingly
strong [Fe II] and Fe II emission spectra in the B and D Weigelt blobs of η Carinae. For our …

Abstract For the Cepheid l Carinae, with a pulsation period of 35.5 days, we have studied
the emission-line fluxes as a function of pulsational phase in order to find out whether we …

Coudé spectra of the nucleus of η Carinae in the ranges of wavelength 3100–4250 Å and H
β–6850 Å have been measured. Wavelengths and estimated intensities are listed in Table …

Quantitative measurements of line parameters in the spectrum of η Carinae are presented
for both the broad and narrow line components. A total of 655 spectral features were …

Wave-lengths and intensity estimates of lines in the spectra of Eta Carinae and RR
Telescopii between 3700 and 8900 A are presented. Both spectra are characterized by …

New Fe II identifications in the infrared spectrum of Page 1 Mon. Not. R. astr. Soc. (1977) 178,
Short Communication, 17P–20P New Fe II identifications in the infrared spectrum of Eta …

Abstract Hubble Space Telescope Space Telescope Imaging Spectrograph (HST STIS) near-
ultraviolet (NUV) echelle spectra reveal complex structure in the sight line toward the …

Results of detailed spectral mapping of the luminous blue variable Eta Car and the
encircling Homunculus are presented. It is shown that the Homunculus is primarily a …