Results 81 to 90 of about 823 (184)

Robust joint modelling of sparsely observed paired functional data

open access: yesCanadian Journal of Statistics, Volume 52, Issue 3, Page 734-754, September 2024.
Abstract A reduced‐rank mixed‐effects model is developed for robust modelling of sparsely observed paired functional data. In this model, the curves for each functional variable are summarized using a few functional principal components, and the association of the two functional variables is modelled through the association of the principal component ...
Huiya Zhou, Xiaomeng Yan, Lan Zhou
wiley   +1 more source

Asteroid (101955) Bennu in the laboratory: Properties of the sample collected by OSIRIS‐REx

open access: yesMeteoritics &Planetary Science, Volume 59, Issue 9, Page 2453-2486, September 2024.
Abstract On September 24, 2023, NASA's OSIRIS‐REx mission dropped a capsule to Earth containing ~120 g of pristine carbonaceous regolith from Bennu. We describe the delivery and initial allocation of this asteroid sample and introduce its bulk physical, chemical, and mineralogical properties from early analyses.
Dante S. Lauretta   +54 more
wiley   +1 more source

Solvatomorphism in a series of copper(II) complexes with the 5‐phenylimidazole/perchlorate system as ligands

open access: yesActa Crystallographica Section B, Volume 80, Issue 4, Page 347-359, August 2024.
The reactions of Cu(ClO4)2·6H2O and L′H in a variety of solvents have provided access to 12 solvatomorphs of the general formula [Cu(ClO4)2(LH)4]·x(solvent); the effect of the solvents on the packing of the complexes is critically discussed.In the course of an investigation of the supramolecular behaviour of copper(II) complexes with the 5 ...
Edward Loukopoulos   +6 more
wiley   +1 more source

Three-dimensional Structure of Incomplete Carbon–Oxygen Detonations in Type Ia Supernovae

open access: yesThe Astrophysical Journal
Carbon–oxygen (CO) detonation with reactions terminating either after burning of ^12 C in the leading ^12 C +  ^12 C reaction or after burning of ^12 C and ^16 O to Si-group elements may occur in the low-density outer layers of exploding white dwarfs and
A. Khokhlov   +8 more
doaj   +1 more source

Neutronization during Type Ia Supernova Simmering

open access: yesThe Astrophysical Journal, 2008
Prior to the incineration of a white dwarf (WD) that makes a Type Ia supernova (SN Ia), the star "simmers" for ~1000 years in a convecting, carbon burning region. We have found that weak interactions during this time increase the neutron excess by an amount that depends on the total quantity of carbon burned prior to the explosion. This contribution is
Piro, Anthony L., Bildsten, Lars
openaire   +2 more sources

SN 2024gy: Multiepoch Spectroscopic Features Suggestive of Delayed Detonation in a Type Ia Supernova

open access: yesThe Astrophysical Journal
We present photometric and spectroscopic observations of SN 2024gy, a Type Ia supernova (SN Ia) exhibiting high-velocity features (HVFs) in its early-time spectra. This SN reaches a peak B -band magnitude of −19.25 ± 0.29 mag and subsequently declines by
Liping Li   +30 more
doaj   +1 more source

SN 2023ehl: A Normal Type Ia Supernova with High-velocity Features

open access: yesThe Astrophysical Journal
SN 2023ehl, a normal Type Ia supernova with a typical decline rate, was discovered in the galaxy UGC 11555 and offers valuable insights into the explosion mechanisms of white dwarfs.
Xiangyun Zeng   +30 more
doaj   +1 more source

The Spatial Distribution of Type Ia Supernovae within Host Galaxies

open access: yesThe Astronomical Journal
We study how type Ia supernovae (SNe Ia) are spatially distributed within their host galaxies, using data taken from the Sloan Digital Sky Survey (SDSS).
Christopher Pritchet   +3 more
doaj   +1 more source

Type Ia supernovae

open access: yes
This is a pre-print of a chapter for the Encyclopedia of Astrophysics (edited by Ilya Mandel, section editor Jeffrey Andrews) to be published by Elsevier as a Reference Module. 18 pages, 7 figures.
openaire   +3 more sources

A Common Origin of Normal Type Ia Supernovae Suggested by the Photometric Diversity

open access: yesThe Astrophysical Journal
In recent years, with the increasing number of type Ia supernovae (SNe Ia) discovered soon after their explosions, a nonnegligible fraction of SNe Ia with early-excess emissions (EExSNe Ia) have been confirmed.
Weiyu Wu   +18 more
doaj   +1 more source

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