Results 221 to 230 of about 74,403 (250)
Multi-omics characterization of diabetic nephropathy in the db/db mouse model of type 2 diabetes. [PDF]
Wang L +6 more
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Coexistence of entanglement-based quantum channels with DWDM classical channels over hollow core fibre in a four node quantum communication network. [PDF]
Clark MJ +12 more
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Distributed multi-parameter quantum metrology with a superconducting quantum network. [PDF]
Zhang J +21 more
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A Search for Trace Amounts of Hydrogen in DB Stars
1991A search for trace amounts of hydrogen in DB stars revealed no hydrogen in a sample of four objects. Upper limits are considerably lower than the quantities of hydrogen found in the DBA stars, stars with He-dominated photospheres and trace quantities of H.
Harry L. Shipman +3 more
openaire +1 more source
Asteroseismology of the DB Star GD 358: Improved Evolutionary Models
2003We have carried out detailed evolutionary calculations of white dwarf models which naturally explain the PG1159-DB-DQ connection. Our evolutionary code (briefly described in Fontaine, Brassard, & Bergeron 2001) was used with the diffusion option turned on.
P. Brassard, G. Fontaine
openaire +1 more source
2013 18th OptoElectronics and Communications Conference held jointly with 2013 International Conference on Photonics in Switching, 2013
Hierarchical modulation with star 8-QAM to upgrade the downlink of PONs is experimentally demonstrated. We confirm 30-dB loss budget in a condition that allows coexistence of standard 10G-EPON ONUs and 30-Gbps DSP-based ONUs.
Noriko Iiyama +3 more
openaire +1 more source
Hierarchical modulation with star 8-QAM to upgrade the downlink of PONs is experimentally demonstrated. We confirm 30-dB loss budget in a condition that allows coexistence of standard 10G-EPON ONUs and 30-Gbps DSP-based ONUs.
Noriko Iiyama +3 more
openaire +1 more source
A new kind of pulsator in the DB valley of white dwarf stars
EAS Publications Series, 2013Recent systematic surveys providing massive datasets of white dwarf stars show that there is still a deficit of a factor of 2.5 in the ratio of white dwarfs showing helium absorption lines to those with hydrogen absorption lines in the temperature range 30 000 K T eff < 45 000 K.
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Group Behaviour of the Pulsating DB White Dwarf Stars
2003We report our progress on a systematic attempt to understand the behaviour of the pulsating DB white dwarfs as a group. Our data base, selected results on individual stars and on pulsational group properties are presented.
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Probing the interior physics of stars through asteroseismology
Reviews of Modern Physics, 2021Conny Aerts
exaly

