Results 131 to 140 of about 82,748 (221)

The fungus Kalmusia longispora is able to cause vascular necrosis on Vitis vinifera. [PDF]

PLoS One, 2021
Karácsony Z, Knapp DG, Lengyel S, Kovács GM, Váczy KZ.   +4 more
europepmc   +1 more source

Characterization of Dwarf Novae Using SDSS Colors

We have developed a method for estimating the orbital periods of dwarf novae from the Sloan Digital Sky Survey (SDSS) colors in quiescence using an artificial neural network.
Uemura, Makoto, Maehara, Hiroyuki, Kato, Taichi   +2 more
core  

UV observations of dwarf novae in quiescence - effects of evaporation?

, 1996
IUE spectra of dwarf novae in quiescence provide information on the inner part of the accretion disk. In the framework of the evaporation model the mass flow of about 10"-"1"1 M_sun/y is understood as accretion via a hot corona above the ...
Meyer-Hofmeister, E. (Max-Planck-Institut fuer Astrophysik, Garching (Germany)), La Dous, C. (Sternwarte Sonneberg (Germany)), Meyer, F., Max-Planck-Institut fuer Astrophysik, Garching (Germany)   +3 more
core  

Cluster Analysis of Presolar Silicon Carbide Grains: Evaluation of Their Classification and Astrophysical Implications. [PDF]

Astrophys J Lett, 2021
Boujibar A, Howell S, Zhang S, Hystad G, Prabhu A, Liu N, Stephan T, Narkar S, Eleish A, Morrison SM, Hazen RM, Nittler LR.   +11 more
europepmc   +1 more source

Binary Parameters for the Recurrent Nova T Coronae Borealis

The Astrophysical Journal
T CrB is among the brightest novae. It is recurrent with outbursts happening approximately every 80 yr. The next outburst is imminent, expected in 2025. The T CrB binary consists of an M4 III red giant (RG) secondary and a white dwarf (WD) primary.
Kenneth H. Hinkle, Pranav Nagarajan, Francis C. Fekel, Joanna Mikołajewska, Oscar Straniero, Matthew W. Muterspaugh   +5 more
doaj   +1 more source

Upper Bound of Ejecta Mass in a Nova Outburst

The Astrophysical Journal
We present the maximum ejecta mass ${({M}_{{\rm{ej}}})}_{{\rm{\max }}}$ and the maximum ratio of ejecta mass and accreted mass ${({M}_{{\rm{ej}}}/{M}_{{\rm{acc}}})}_{{\rm{\max }}}$ of a nova for various white dwarf (WD) masses ( M _WD  = 0.6–1.38 M _ ...
Izumi Hachisu, Mariko Kato
doaj   +1 more source

An evolutionary system of mineralogy. Part I: Stellar mineralogy (>13 to 4.6 Ga). [PDF]

Am Mineral, 2020
Hazen RM, Morrison SM.
europepmc   +1 more source

A Nova Scotian dwarf shadbush

, 1948
(Uploaded by Plazi from the Biodiversity Heritage Library) No abstract provided.
openaire   +2 more sources

A National Catalogue of Viruses Associated with Indigenous Species Reveals High-Throughput Sequencing as a Driver of Indigenous Virus Discovery. [PDF]

Viruses, 2022
Robson M, Chooi KM, Blouin AG, Knight S, MacDiarmid RM.   +4 more
europepmc   +1 more source

Diversity, Distribution, Systematics and Conservation Status of Podocarpaceae. [PDF]

Plants (Basel), 2023
Khan R, Hill RS, Liu J, Biffin E.
europepmc   +1 more source