Results 71 to 80 of about 493,128 (267)

POSITIVE AND NEGATIVE SUPERHUMPS OF THE DWARF NOVA MN DRA

open access: yesOdessa Astronomical Publications, 2010
We present the result of O–C analysis of the dwarf nova MN Dra. It is based on the multi-site photometric observations that were made over 77 nights in August – November, 2009. The total exposure was 433 hours.
D. A. Samsonov   +9 more
doaj   +1 more source

Erupting Cataclysmic Variable Stars in the Nearest Globular Cluster, NGC 6397: Intermediate Polars?

open access: yes, 2005
NGC 6397 is the closest globular cluster, and hence the ideal place to search for faint stellar populations such as cataclysmic variables (CVs). HST and Chandra observers have identified nine certain and likely CVs in this nearby cluster, including ...
A. Dieball   +9 more
core   +2 more sources

The nature of dwarf nova outbursts [PDF]

open access: yes, 2000
We show that if the dwarf-nova disc instability model includes the effects of heating by stream impact and tidal torque dissipation in the outer disc, the calculated properties of dwarf-nova outbursts change considerably, and several notorious ...
Armitage   +47 more
core   +4 more sources

The Massive CO White Dwarf in the Symbiotic Recurrent Nova RS Ophiuchi [PDF]

open access: yes, 2017
If accreting white dwarfs (WDs) in binary systems are to produce type Ia supernovae (SNe Ia), they must grow to nearly the Chandrasekhar mass and ignite carbon burning.
J. Mikołajewska, M. Shara
semanticscholar   +1 more source

Hidden lineages in the African Sky Islands: A taxonomic reevaluation of Afrocarduus (Compositae)

open access: yesJournal of Systematics and Evolution, EarlyView.
Species delimitation is crucial for biodiversity studies. Using Hyb‐Seq and phylogenomics, we reassessed Afrocarduus, endemic to Afromontane and Afroalpine regions, uncovering 16 evolutionary lineages (2.3 Mya). Morphological data support their distinctiveness, with acaulescence evolving independently twice. The traditionally broad A.
Lucía D. Moreyra   +9 more
wiley   +1 more source

SPECTROSCOPIC MONITORING OF NOVA VULPECULAE 2007 (V458 Vul)

open access: yesOdessa Astronomical Publications, 2008
We present results of the spectroscopic monitoring of the peculiar nova V458 Vul during eleven months. At the early decline of the brightness the nova transformed from Fe II to the He/N type.
T. N. Tarasova
doaj   +1 more source

Long-term photometry of the eclipsing dwarf nova V893 Scorpii - Orbital period, oscillations, and a possible giant planet [PDF]

open access: yes, 2014
The cataclysmic variable V893 Sco is an eclipsing dwarf nova which, apart from outbursts with comparatively low amplitudes, exhibits a particularly strong variability during quiescence on timescales of days to seconds.The present study aims to update the
A. Bruch
semanticscholar   +1 more source

Nations as Natural Families: From Kin Selection to Multilevel Selection

open access: yesNations and Nationalism, EarlyView.
ABSTRACT In nationalism studies, nations are often viewed as artificial constructs. By contrast, many sociobiologists see nations as natural families or kin groups. They explain altruism and shared ancestry among co‐nationals through kin selection theory, which accounts for altruism towards close genetic relatives. In this article, we refine and deepen
Filipe Nobre Faria, Sandra Dzenis
wiley   +1 more source

Extensive photometry of the WZ Sge-type dwarf nova V455 And (HS2331+3905): detection of negative superhumps and coherence features of the short-period oscillations [PDF]

open access: yes, 2015
We report the results of photometry of the WZ Sge-type dwarf nova V455 And. Observations were obtained over 19 nights in 2013 and 2014. The total duration of the observations was 96 h.
Kozhevnikov, V. P.
core   +1 more source

The Kukarkin-Parenago Relation for Dwarf Novae and Novae [PDF]

open access: yesAstrophysics and Space Science, 1987
AbstractThe period-amplitude relation and the period-energy relation for dwarf novae and novae are discussed. The total outbursts energy is shown to be a more suitable characteristic of the outburst than its amplitude.
openaire   +1 more source

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