Zobrazeno 1 - 10
of 121
pro vyhledávání: '"Katherine Shepard"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Katherine Shepard, Douglas R. Gies, Gail H. Schaefer, Narsireddy Anugu, Fabien R. Baron, Cyprien Lanthermann, John D. Monnier, Stefan Kraus, Theo ten Brummelaar
Publikováno v:
The Astrophysical Journal, Vol 977, Iss 2, p 236 (2024)
W Serpentis is an eclipsing binary system and the prototype of the Serpentid class of variable stars. These are interacting binaries experiencing intense mass transfer and mass loss. However, the identities and properties of both stars in W Ser remai
Externí odkaz:
https://doaj.org/article/3beb98d6023b4f49bc5e8473337f7b3c
Publikováno v:
In Ecological Modelling 24 July 2017 356:59-72
Publikováno v:
In Ecological Modelling 10 February 2013 250:214-234
Autor:
Caleb Taylor, Melissa M. Baustian, Erin P. Kiskaddon, Katherine Shepard Watkins, Shaye E. Sable, Megan K. La Peyre
Publikováno v:
Ecological Indicators, Vol 133, Iss, Pp 108404-(2021)
Long-term fisheries-independent sampling data inform population status and trends of species-specific biomass and are often used to drive biomass-based food web models such as the Comprehensive Aquatic Systems Model (CASM). Indicators such as total b
Publikováno v:
Astrophysical Journal, 931:931. IOP Publishing Ltd.
We present a spectroscopic analysis of the most rapidly rotating stars currently known, VFTS 102 ($v_{e} \sin i = 649 \pm 52$ km s$^{-1}$; O9: Vnnne+) and VFTS 285 ($v_{e} \sin i = 610 \pm 41$ km s$^{-1}$; O7.5: Vnnn), both members of the 30 Dor comp
HD 93521 is a massive, rapidly rotating star that is located about 1 kpc above the Galactic disk, and the evolutionary age for its estimated mass is much less than the time-of-flight if it was ejected from the disk. Here we present a re-assessment of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9f9f9b8397c00e8d68ca19cca065995d
Autor:
Kathryn V. Lester, Coralie Neiner, Gregg A. Wade, J. Dunham, Douglas R. Gies, Katherine Shepard, Luqian Wang, David W. Dunham, Andrew Couperus
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2020, 902 (1), pp.25. ⟨10.3847/1538-4357/abb372⟩
The Astrophysical Journal, American Astronomical Society, 2020, 902 (1), pp.25. ⟨10.3847/1538-4357/abb372⟩
Mass transfer in an interacting binary will often strip the mass donor of its entire envelope and spin up the mass gainer to near critical rotation. The nearby B-type star Regulus represents a binary in the post-mass transfer stage: it is a rapid rot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b0b1cc8fa003181f4b1b331e5fc0bbf
http://arxiv.org/abs/2009.02409
http://arxiv.org/abs/2009.02409
Publikováno v:
Ecological Modelling. 356:59-72
The accuracy of spatially-explicit individual-based models (IBMs) often depends on the realistic simulation of the movement of organisms, which is especially challenging when movement cues (e.g., environmental conditions; prey and predator abundances
Autor:
Kiva L. Oken, Elizabeth E. Holmes, Eric J. Ward, Katherine Shepard Watkins, Mark D. Scheuerell, Kenneth A. Rose, Shaye E. Sable
Publikováno v:
Environmental monitoring and assessment, vol 190, iss 9
Quantifying the impacts of disturbances such as oil spills on marine species can be challenging. Natural environmental variability, human responses to the disturbance (e.g., fisheries closures), the complex life histories of the species being monitor