New insights into classical novae
L Chomiuk, BD Metzger, KJ Shen - Annual Review of Astronomy …, 2021 - annualreviews.org
We survey our understanding of classical novae—nonterminal, thermonuclear eruptions on
the surfaces of white dwarfs in binary systems. The recent and unexpected discovery of GeV …
the surfaces of white dwarfs in binary systems. The recent and unexpected discovery of GeV …
Observational constraints on the feeding of supermassive black holes
T Storchi-Bergmann, A Schnorr-Müller - Nature Astronomy, 2019 - nature.com
Supermassive black holes grow at the centre of galaxies in consonance with them. In this
Review Article, we discuss the mass-feeding mechanisms that lead to this growth in active …
Review Article, we discuss the mass-feeding mechanisms that lead to this growth in active …
The messy death of a multiple star system and the resulting planetary nebula as observed by JWST
Planetary nebulae—the ejected envelopes of red giant stars—provide us with a history of
the last, mass-losing phases of 90% of stars initially more massive than the Sun. Here we …
the last, mass-losing phases of 90% of stars initially more massive than the Sun. Here we …
[HTML][HTML] ALMA data suggest the presence of spiral structure in the inner wind of CW Leonis
Context. Evolved low-mass stars lose a significant fraction of their mass through stellar
winds. While the overall morphology of the stellar wind structure during the asymptotic giant …
winds. While the overall morphology of the stellar wind structure during the asymptotic giant …
Study of 2021 outburst of the recurrent nova RS Ophiuchi: Photoionization and morphokinematic modelling
We present the evolution of the optical spectra of the 2021 outburst of RS Ophiuchi (RS Oph)
over about a month after the outburst. The spectral evolution is similar to the previous …
over about a month after the outburst. The spectral evolution is similar to the previous …
Submillimeter-wave emission of three Galactic red novae: cool molecular outflows produced by stellar mergers
T Kamiński, W Steffen, R Tylenda, KH Young… - Astronomy & …, 2018 - aanda.org
Red novae are optical transients erupting at luminosities typically higher than those of
classical novae. Their outbursts are believed to be caused by stellar mergers. We present …
classical novae. Their outbursts are believed to be caused by stellar mergers. We present …
Study of the fastest classical nova, V1674 Her: photoionization and morpho-kinemetic model analysis
We present the results of the investigation of the nova V1674 Her (2021), recognized as the
swiftest classical nova, with t 2∼ 0.90 d. The distance to the nova is estimated to be 4.97 …
swiftest classical nova, with t 2∼ 0.90 d. The distance to the nova is estimated to be 4.97 …
[HTML][HTML] V838 Monocerotis as seen by ALMA: A remnant of a binary merger in a triple system
T Kamiński, R Tylenda, A Kiljan, M Schmidt… - Astronomy & …, 2021 - aanda.org
Context. V838 Mon erupted in 2002, quickly becoming the prototype of a new type of stellar
eruption known today as the (luminous) red nova. Red nova outbursts are thought to be …
eruption known today as the (luminous) red nova. Red nova outbursts are thought to be …
Visualization in astrophysics: Developing new methods, discovering our universe, and educating the earth
F Lan, M Young, L Anderson… - Computer graphics …, 2021 - Wiley Online Library
We present a state‐of‐the‐art report on visualization in astrophysics. We survey
representative papers from both astrophysics and visualization and provide a taxonomy of …
representative papers from both astrophysics and visualization and provide a taxonomy of …
Optical morphology, inclination, and expansion velocity of the ejected shell of Nova Monocerotis 2012
The morphology of the ejected shell of the He/N Nova Monocerotis 2012 outburst was
studied in detail. Synthetic line profile spectra were compared to the [O iii] 4959, 5007 Å …
studied in detail. Synthetic line profile spectra were compared to the [O iii] 4959, 5007 Å …