Results 81 to 90 of about 9,193 (307)
SDSS white dwarf mass distribution at low effective temperatures [PDF]
, 2009 The DA white dwarfs in the Sloan Digital Sky Survey, as analyzed in the papers for Data Releases 1 and 4, show an increase in surface gravity towards lower effective temperatures below 11500 K.
Kleinman, Scot J. +5 more
core +1 more source
Archaeology in Oceania, EarlyView.ABSTRACT In this paper we report on faunal remains recovered from a legacy archaeological excavation undertaken in the rockshelter entrance of Waribruk (New Guinea II Cave), a GunaiKurnai site located on the west bank of the Snowy River, East Gippsland, southeastern Australia.
Matthew C. McDowell +7 more
wiley +1 more source
A Detailed Model Atmosphere Analysis of Hot White Dwarfs in DESI DR1
The Astrophysical JournalWe present a detailed model atmosphere analysis of hot white dwarfs in the Dark Energy Spectroscopic Instrument (DESI) Data Release 1. Our sample includes 19,321 unique targets with G _BP − G _RP ≤ 0.
Mukremin Kilic +8 more
doaj +1 more source
Astronomy & AstrophysicsContext. The latest Gaia data release provides astrometric measurements for 1.8 billion sources and low-resolution spectra for 220 million sources, including approximately 100 000 white dwarfs.
García-Zamora Enrique Miguel +3 more
doaj +1 more source
Heat Stress in Quail: Impacts on Health and Productivity, and Mitigation Strategies
Animal Research and One Health, EarlyView.Heat stress disrupts physiological homeostasis in quail, inducing oxidative stress, immune dysregulation, and metabolic imbalance, which impair growth, reproduction, product quality, and welfare. Integrating nutritional, environmental, and genetic–epigenetic strategies enhances thermotolerance, sustains productivity, and supports climate‐smart quail ...
T. A. Eletu +6 more
wiley +1 more source
Measuring the Mass–Radius Relation of White Dwarfs Using Wide Binaries
The Astrophysical JournalMeasuring the mass–radius relation of individual white dwarfs is an empirically challenging task that has been performed for only a few dozen stars. We measure the white dwarf mass–radius relation using the gravitational redshifts and radii of 135 white ...
Stefan Arseneau +12 more
doaj +1 more source
On the Structure of Pre-White Dwarfs [PDF]
International Astronomical Union Colloquium, 1989 White dwarfs (WD) are the final configurations of all stars up to initial masses between 5 and 9 M⊙. Two feeder channels for the creation of single WDs can be distinguished: Either evolution through the asymptotic giant branch (AGB) and the following planetary-nebula (PN) phase, or evolution from the horizontal branch through the hot subdwarf region ...
D. Schönberner, R. Tylenda
openaire +1 more source
Snow White in 1930s Britain [PDF]
, 2010 This is the definitive version of the article as published by Edinburgh University Press in Journal of British Cinema and Television. Volume 7, Page 183-199 DOI 10.3366/jbctv.2010.0001 http://www.euppublishing.com/doi/abs/10.3366/jbctv.2010 ...
Annette Kuhn, KUHN, AF
core +1 more source
Essential work, invisible workers: The role of digital curation in COVID‐19 Open Science
Journal of the Association for Information Science and Technology, Volume 76, Issue 4, Page 703-717, April 2025.Abstract In this paper, we examine the role digital curation practices and practitioners played in facilitating open science (OS) initiatives amid the COVID‐19 pandemic. In Summer 2023, we conducted a content analysis of available information regarding 50 OS initiatives that emerged—or substantially shifted their focus—between 2020 and 2022 to address ...
Irene V. Pasquetto +2 more
wiley +1 more source
Derivation of the Stellar Formation History from White Dwarfs in the Solar Neighborhood [PDF]
, 2015 The study of volume complete samples in the solar neighborhood is a powerful technique to learn about the stellar formation history and the initial mass function. We probe the local formation history from the volume complete sample of white dwarfs within
Soderblom, D. R. +4 more
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