Add to ORKGMajor 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 observational record. The simplest, but unproven, explanation is a rapid decrease in the wind density
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
The periodic spectroscopic events in η Carinae are now well established and occur near the periastro...
At the heart of Eta Carinae's spectacular bipolar ``Homunculus" nebula lies an extremely luminous (5...
Major stellar-wind emission features in the spectrum of η Car have recently decreased by factors of ...
We monitored Eta Carinae with the Hubble Space Telescope WFPC2 and Gemini GMOS throughout the 2009 s...
Recent work suggests that the mass-loss rate of the primary star Eta-A in the massive colliding wind...
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
Over the entire 20th century, Eta Carinae (\ec) has displayed a unique spectrum, which recently has ...
We report on the N II λλ5668-5712 emission and absorption lines in the spectrum of η Carinae. Spectr...
Eta Carinae, the closest, active, massive binary containing a highly unstable Luminous Blue Variable...
The Homunculus reflection nebula around eta Carinae provides a rare opportunity to observe the spect...
The supernova imposter Eta Carinae and its surrounding Homunculus reflection nebula have been of gre...
We have analyzed high spatial, moderate spectral resolution observations of Eta Carinae obtained wit...
A series of three Hubble Space Telescope Space Telescope Imaging Spectrograph (HST/STIS) spectroscop...
Eta Carinae (Eta Car), its interacting winds and historical ejecta provide an unique astrophysical l...
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
The periodic spectroscopic events in η Carinae are now well established and occur near the periastro...
At the heart of Eta Carinae's spectacular bipolar ``Homunculus" nebula lies an extremely luminous (5...
Major stellar-wind emission features in the spectrum of η Car have recently decreased by factors of ...
We monitored Eta Carinae with the Hubble Space Telescope WFPC2 and Gemini GMOS throughout the 2009 s...
Recent work suggests that the mass-loss rate of the primary star Eta-A in the massive colliding wind...
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
Over the entire 20th century, Eta Carinae (\ec) has displayed a unique spectrum, which recently has ...
We report on the N II λλ5668-5712 emission and absorption lines in the spectrum of η Carinae. Spectr...
Eta Carinae, the closest, active, massive binary containing a highly unstable Luminous Blue Variable...
The Homunculus reflection nebula around eta Carinae provides a rare opportunity to observe the spect...
The supernova imposter Eta Carinae and its surrounding Homunculus reflection nebula have been of gre...
We have analyzed high spatial, moderate spectral resolution observations of Eta Carinae obtained wit...
A series of three Hubble Space Telescope Space Telescope Imaging Spectrograph (HST/STIS) spectroscop...
Eta Carinae (Eta Car), its interacting winds and historical ejecta provide an unique astrophysical l...
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
The periodic spectroscopic events in η Carinae are now well established and occur near the periastro...
At the heart of Eta Carinae's spectacular bipolar ``Homunculus" nebula lies an extremely luminous (5...