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993 results for “T Dwarfs”

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zenodo36/100

The C-flame Quenching by Convective Boundary Mixing in Super-AGB Stars and the Formation of Hybrid C/O/Ne White Dwarfs and SN Progenitors

<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/#abs/2013ApJ...772...37D/abstract">Denissenkov et al. (2013)</a>. MESA version 4631.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.1088/0004-637X/772/1/37">10.1088/0004-637X/772/1/37</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Polluting white dwarfs with perturbed exo-comets

<p>MESA inlists associated with <a href="https://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.2750C/abstract">Caiazzo et al. (2017)</a>. MESA version 5456.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.1093/mnras/stx1036">10.1093/mnras/stx1036</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Effective temperatures of cataclysmic-variable white dwarfs as a probe of their evolution

<p>MESA inlists associated with&nbsp;<a href="https://ui.adsabs.harvard.edu/?#abs/2017MNRAS.466.2855P">Effective temperatures of cataclysmic-variable white dwarfs as a probe of their evolution</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Tidal dissipation and evolution of white dwarfs around massive black holes: an eccentric path to tidal disruption

<p>MESA inlists associated with&nbsp;<a href="https://ui.adsabs.harvard.edu/?#abs/2017MNRAS.468.2296V">Tidal dissipation and evolution of white dwarfs around massive black holes: an eccentric path to tidal disruption</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Novel modelling of ultracompact X-ray binary evolution - stable mass transfer from white dwarfs to neutron stars

<p>MESA inlists associated with&nbsp;<a href="https://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L...6S/abstract">Novel modelling of ultracompact X-ray binary evolution - stable mass transfer from white dwarfs to neutron stars</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

New full evolutionary sequences of H- and He-atmosphere massive white dwarf stars using MESA

<p>MESA inlists associated with&nbsp;<a href="https://ui.adsabs.harvard.edu/?#abs/2018MNRAS.480.1547L">New full evolutionary sequences of H- and He-atmosphere massive white dwarf stars using MESA</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Carbon Shell or Core Ignitions in White Dwarfs Accreting from Helium Stars

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2016ApJ...821...28B">Brooks et al. (2016)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/0004-637X/821/1/28">10.3847/0004-637X/821/1/28</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Fast and Luminous Transients from the Explosions of Long-lived Massive White Dwarf Merger Remnants

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2017ApJ...850..127B">Brooks et al. (2017)</a>. MESA version 9793.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/1538-4357/aa9568">10.3847/1538-4357/aa9568</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Properties of Carbon-Oxygen White Dwarfs From Monte Carlo Stellar Models

<p>MESA inlists and models associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2016ApJ...823...46F">Fields et al. (2016)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/0004-637X/823/1/46">10.3847/0004-637X/823/1/46</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

PTF1 J082340.04+081936.5: A Hot Subdwarf B Star with a Low-mass White Dwarf Companion in an 87-minute Orbit

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2017ApJ...835..131K">Kupfer et al. (2017)</a>. MESA version 8118.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/1538-4357/835/2/131">10.3847/1538-4357/835/2/131</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Accretion-induced Collapse from Helium Star + White Dwarf Binaries

<p>MESA inlists and run_star_extras associated with <a href="https://ui.adsabs.harvard.edu/?#abs/2017ApJ...843..151B">Brooks et al. (2017)</a>. MESA version 7624.</p> <p>Publication DOI:&nbsp;<a href="https://doi.org/10.3847/1538-4357/aa79a6">10.3847/1538-4357/aa79a6</a></p>

opencc-by-4.0Mar 2019View details →
zenodo36/100

Stellar Density Profiles of Dwarf Spheroidal Galaxies: Posterior Distributions

<p>This archive contains samples from the posterior distributions of our 3-plummer, 1-plummer, 3-steeper and 1-steeper fits for 38 dwarf spheroidal galaxies.</p>

opencc-by-4.0Oct 2019View details →
zenodo36/100

GCM simulations of Earth-like M- and K-dwarf planets

<p>Simulations are described in papers:</p> <ul> <li> <div>Lobo, A. H., Shields, A. L., Palubski, I. Z., &amp; Wolf, E. (2023). <strong>Terminator Habitability: The Case for Limited Water Availability on M-dwarf Planets</strong>. <em>The Astrophysical Journal</em>, <em>945</em>(2), 161. https://doi.org/10.3847/1538-4357/aca970</div> </li> <li>Lobo, A. H., Shields, A. L., (in press, 2024). <strong>Climate Regimes Across the Habitable Zone: a Comparison of Synchronous Rocky M- and K-dwarf Planets</strong>. <em>The Astrophysical Journal.&nbsp;</em></li> </ul> <p>&nbsp;</p>

opencc-by-4.0Aug 2024View details →
zenodo36/100

The Ultracool Dwarf Companion catalouge

<p>This dataset contains the catalogue accompanying the paper "The &nbsp;Gaia Ultracool<br>&nbsp; Dwarf Sample -- V: The Ultracool Dwarf Companion catalogue" by Sayan Baig et al., accepted by MNRAS in July 2024.</p>

opencc-by-4.0Aug 2024View details →
zenodo36/100

Stellar Parameter Estimation for Half a Million M Dwarfs based on Cycle-StarNet

Open the record for dataset details and reuse information.

opencc-by-4.0Aug 2024View details →
zenodo36/100

Model Fit Figures for: The 100 pc White Dwarf Sample in the SDSS Footprint II. A New Look at the Spectral Evolution of White Dwarfs

<p>Figures for the model atmosphere fits to the spectroscopically confirmed white dwarfs in the 100 pc sample and the SDSS footprint (<span>arXiv:2412.04611).&nbsp;</span></p>

opencc-by-4.0Sep 2024View details →
zenodo36/100

Blue large-amplitude pulsators formed from the merger of low-mass white dwarfs

<p>Here you will find the files necessary to reproduce the simulations from our work using the MESA (version 23.05.01), GYRE (version 6.0.1), and COSMIC (version 3.4.10) codes.</p>

opencc-by-4.0Sep 2024View details →
dryad36/100

Data from: Diversity and composition of viral communities: coinfection of barley and cereal yellow dwarf viruses in California grasslands

Most species host multiple pathogens, yet field studies rarely examine the processes determining pathogen diversity within a single host or the effects of coinfection on pathogen dynamics in natural systems. Coinfection can affect pathogen transmission and virulence. In turn, coinfection can be regulated within hosts by interactions such as cross-protective immunity or at broader spatial scales via vector distributions. Using a general model, we demonstrate that coinfection by a group of vectored pathogens is highest with abundant generalist vectors and weak cross-protection and coinfection- induced mortality. Using these predictions, we investigate the distribution of five coexisting aphid-vectored, viral pathogens (barley and cereal yellow dwarf luteoviruses and poleroviruses) in a native perennial grass (Elymus glaucus) in both space (700 km) and time (4 years). Observed coinfection rates were much higher than expected at random, suggesting that within-host processes exerted weak effects on within-host pathogen diversity. Covariance among viruses in space and time was highest for viral species sharing a vector. Temporal correlation arose from the synchronous invasion of two viruses transmitted by a shared aphid species. On the basis of our modeling and empirical results, we expect that factors external to individual hosts may affect the coinfection dynamics in other communities hosting vectored pathogens.

opencc-zeroDec 2017View details →
zenodo36/100

Fig. 1. Scoloplax baskini, INPA 28658 in Scoloplax baskini: a new spiny dwarf catfish from rio Aripuanã, Amazonas, Brazil (Loricarioidei: Scoloplacidae)

Fig. 1. Scoloplax baskini, INPA 28658, holotype, 14.4 mm SL. Photo by R. R. de Oliveira.

opencc-by-4.0Dec 2008View details →
zenodo36/100

Multidimensional Parameter Study of Double Detonation Type Ia Supernovae Originating from Thin Helium Shell White Dwarfs

<p>This dataset provides the end-state ejecta data for each of the simulations from Boos et al. 2021, along with condensed versions for use in radiative transfer calculations.</p>

opencc-by-4.0Sep 2021View details →

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Allen Brain Atlas

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neuroscienceopenDocumentation, web resources, and API references are available online.
Last verified 2026-04-30Open record

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behavioral-neuroscienceopenThe DataShare record exposes download links for annotations, documentation, license text, and the zipped per-snippet data directory.
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DANDI Archive for NWB datasets

DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.

dandi-nwb
electrophysiologyopenPublished Dandiset metadata and archive endpoints are available through the production DANDI API.
Last verified 2026-04-30Open record

International Brain Laboratory public data

The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.

ibl
behavioral-neuroscienceopenPublic sessions can be searched and loaded from the IBL public data server through ONE.
Last verified 2026-04-29Open record

OpenNeuro

OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.

openneuro
neuroscienceopenPublished datasets are available on demand over the internet.
Last verified 2026-04-29Open record

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