We have discovered a conspicuous unidentified variable feature near 6307 Å in the
spectrum of η Carinae that is spatially unresolved from the central star and its wind (r≲ 200 …

We report on the N ii λλ5668–5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …

Two years ago, a workshop entitled h Carinae at the Millennium (1999, ASP Conf. Ser. 179,
ed. JA Morse, RM Humphreys, & A. Damineli [San Francisco: ASP]) was held to evaluate the …

The motivations for a meeting on h Carinae at this time were many–the remarkable
discoveries in the past few years about the spectra of the star and its ejecta, the bipolar …

We present high spectral resolution echelle observations of the Balmer line variations during
the 2003.5" spectroscopic event" of η Carinae. Spectra have been recorded of both η Car …

The first far ultraviolet high spectral resolution observations of ij Carinae were obtained with
the Far Ultraviolet Spectroscopic Explorer satellite in February and March 2000. The …

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 …

Major stellar-wind emission features in the spectrum of η Car have recently decreased by
factors of order 2 relative to the continuum. This is unprecedented in the modern …

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 …

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 …