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Nonthermal particles and photons in starburst regions and superbubbles
AM Bykov - The Astronomy and Astrophysics Review, 2014 - Springer
Starforming factories in galaxies produce compact clusters and loose associations of young
massive stars. Fast radiation-driven winds and supernovae input their huge kinetic power …
massive stars. Fast radiation-driven winds and supernovae input their huge kinetic power …
First light for GRAVITY: Phase referencing optical interferometry for the Very Large Telescope Interferometer
GRAVITY is a new instrument to coherently combine the light of the European Southern
Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 …
Observatory Very Large Telescope Interferometer to form a telescope with an equivalent 130 …
On variations of pre-supernova model properties
R Farmer, CE Fields, I Petermann… - The Astrophysical …, 2016 - iopscience.iop.org
We explore the variation in single-star 15–30 M, nonrotating, solar metallicity, pre-
supernova MESA models that is due to changes in the number of isotopes in a fully coupled …
supernova MESA models that is due to changes in the number of isotopes in a fully coupled …
Supernova remnants of red supergiants: From barrels to loops
Core-collapse (CC) supernova remnants (SNRs) are the nebular leftovers of defunct
massive stars that died during a supernova explosion, mostly while undergoing the red …
massive stars that died during a supernova explosion, mostly while undergoing the red …
Scientific problems addressed by the Spektr-UV space project (world space Observatory—Ultraviolet)
AA Boyarchuk, BM Shustov, IS Savanov, ME Sachkov… - Astronomy Reports, 2016 - Springer
The article presents a review of scientific problems and methods of ultraviolet astronomy,
focusing on perspective scientific problems (directions) whose solution requires UV space …
focusing on perspective scientific problems (directions) whose solution requires UV space …
Non-thermal X-rays from colliding wind shock acceleration in the massive binary Eta Carinae
Cosmic-ray acceleration has been a long-standing mystery, and, despite more than a
century of study, we still do not have a complete census of acceleration mechanisms. The …
century of study, we still do not have a complete census of acceleration mechanisms. The …
Simulating the formation of η Carinae's surrounding nebula through unstable triple evolution and stellar merger-induced eruption
ABSTRACT η Carinae is an extraordinary massive star famous for its 19th century Great
Eruption and the surrounding Homunculus nebula ejected in that event. The cause of this …
Eruption and the surrounding Homunculus nebula ejected in that event. The cause of this …
He II λ4686 EMISSION FROM THE MASSIVE BINARY SYSTEM IN η CAR: CONSTRAINTS TO THE ORBITAL ELEMENTS AND THE NATURE OF THE PERIODIC …
ABSTRACT Eta Carinae (η Car) is an extremely massive binary system in which rapid
spectrum variations occur near periastron. Most notably, near periastron the He ii λ4686 line …
spectrum variations occur near periastron. Most notably, near periastron the He ii λ4686 line …
The first full orbit of η Carinae seen by Fermi
Aims. The binary system η Carinae has completed its first 5.54 y orbit since the beginning of
science operation of the Fermi Large Area Telescope (LAT). We are now able to investigate …
science operation of the Fermi Large Area Telescope (LAT). We are now able to investigate …
The 2014 X-ray minimum of η Carinae as seen by Swift
MF Corcoran, J Liburd, D Morris… - The Astrophysical …, 2017 - iopscience.iop.org
We report on Swift X-ray Telescope observations of Eta Carinae (η Car), an extremely
massive, long-period, highly eccentric binary obtained during the 2014.6 X-ray …
massive, long-period, highly eccentric binary obtained during the 2014.6 X-ray …