Eta Carinae's inner ejecta are dominated observationally by the bright Weigelt blobs and
their famously rich spectra of nebular emission and absorption lines. They are dense (ne∼ …

This contribution presented high-resolution numerical simulations of the colliding wind
system η Carinae, showing accretion of the primary wind onto the secondary star close to …

ABSTRACT The interacting binary Eta Carinae remains one of the most enigmatic massive
stars in our Galaxy despite over four centuries of observations. In this work, its light curve …

During its first 2 years of operation, the gamma-ray AGILE satellite accumulated an
extensive dataset for the Galactic plane. The data have been monitored for transient sources …

Eta Carinae is the most massive active binary within 10,000 light-years. While famous for the
largest non-terminal stellar explosion ever recorded, observations reveal a supermassive …

The present work discusses astronomical site survey reports on dust content, vertical
distribution of atmospheric turbulence, precipitable water vapor (PWV), surface and upper …

Eta Carinae, the closest, active, massive binary containing a highly unstable LBV, exhibits
expanding, compressed wind shells, seen in emission, that are spatially and spectrally …

We have monitored the massive binary star $\eta $ Carinae with the CTIO/SMARTS 1.5~ m
telescope and CHIRON spectrograph from the previous apastron passage of the system …

We show that recent observations of He I and N II lines of $\eta $ Carinae may provide
support for an orbital orientation where the secondary star is closest to us at periastron …

The evolution of massive stars, as well as their endpoints as supernovae (SNe), is important
both in astrophysics and cosmology. While tremendous progress towards an understanding …