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
Aims. Eta Car's ultra-violet, optical, and X-ray light curves and its spectrum suggest a physical ch...
The periodic spectroscopic events in eta Carinae are now well established and occur near the periast...
We present narrowband images of eta Carinae in the light of [O III] 5007 obtained with HST/WFPC2, as...
Major stellar-wind emission features in the spectrum of η Car have recently decreased by factors of ...
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
Eta Carinae, the closest, active, massive binary containing a highly unstable Luminous Blue Variable...
Artículo de publicación ISIAims. Every 5.5 years, eta Car's light curve and spectrum change remarkab...
At the heart of Eta Carinae's spectacular bipolar ``Homunculus" nebula lies an extremely luminous (5...
Artículo de publicación ISIAims. Every 5.5 years, eta Car's light curve and spectrum change remarkab...
We present new high angular resolution observations at near-IR wavelengths of the core of the Lumino...
We present new high angular resolution observations at near-IR wavelengths of the core of the Lu...
FUV spectra of eta Car, recorded across two decades with HST/STIS, document multiple changes in reso...
FUV spectra of eta Car, recorded across two decades with HST/STIS, document multiple changes in reso...
Recent work suggests that the mass-loss rate of the primary star Eta-A in the massive colliding wind...
Aims. Eta Car's ultra-violet, optical, and X-ray light curves and its spectrum suggest a physical ch...
The periodic spectroscopic events in eta Carinae are now well established and occur near the periast...
We present narrowband images of eta Carinae in the light of [O III] 5007 obtained with HST/WFPC2, as...
Major stellar-wind emission features in the spectrum of η Car have recently decreased by factors of ...
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
Eta Carinae (η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components....
Eta Carinae, the closest, active, massive binary containing a highly unstable Luminous Blue Variable...
Artículo de publicación ISIAims. Every 5.5 years, eta Car's light curve and spectrum change remarkab...
At the heart of Eta Carinae's spectacular bipolar ``Homunculus" nebula lies an extremely luminous (5...
Artículo de publicación ISIAims. Every 5.5 years, eta Car's light curve and spectrum change remarkab...
We present new high angular resolution observations at near-IR wavelengths of the core of the Lumino...
We present new high angular resolution observations at near-IR wavelengths of the core of the Lu...
FUV spectra of eta Car, recorded across two decades with HST/STIS, document multiple changes in reso...
FUV spectra of eta Car, recorded across two decades with HST/STIS, document multiple changes in reso...
Recent work suggests that the mass-loss rate of the primary star Eta-A in the massive colliding wind...
Aims. Eta Car's ultra-violet, optical, and X-ray light curves and its spectrum suggest a physical ch...
The periodic spectroscopic events in eta Carinae are now well established and occur near the periast...
We present narrowband images of eta Carinae in the light of [O III] 5007 obtained with HST/WFPC2, as...