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Predicting Major Depression Among Diverse Online Gamers: The Role of Internet Addiction and Spirituality

Journal of Addictions &Offender Counseling, EarlyView.
ABSTRACT This study analyzed whether religious or spiritual affiliation and therapy enrollment protect against symptoms meeting Major Depressive Disorder criteria beyond demographic, Internet addiction, and described therapy enrollment. Findings illustrated one risk factor and one protective factor associated with experiencing symptoms that meet Major ...
Lindsay A. Lundeen, John R. McCall
wiley   +1 more source

The We‐Relationship as a Key to Addressing Dementia‐Related Ambiguous Loss

Journal of Applied Philosophy, EarlyView.
ABSTRACT Pauline Boss describes the challenges faced by people caring for family members with dementia in terms of ambiguous loss – a condition in which the physical presence of the person with dementia coexists with their psychological absence. This article proposes the concept of we‐relationship as a key to addressing dementia‐related ambiguous loss.
Takuya Niikawa, Xue Li
wiley   +1 more source

Cold brown dwarfs with WISE: Y dwarfs and the field mass function

Astronomische Nachrichten, 2013
AbstractThe discovery of a new spectral class – the Y dwarfs – by NASA's Wide‐field Infrared Survey Explorer has enabled researchers to study the physics of the coldest brown dwarfs and to determine the prevalence of brown dwarfs in the Milky Way. The boundary between T dwarfs and Y dwarfs roughly coincides with the location where the J – H colors of ...
Kirkpatrick, J. D.
openaire   +3 more sources

Atmospheres of brown dwarfs

Astronomy and Astrophysics Review, 2014
ChH highlights financial support of the European Community under the FP7 by an ERC starting grant. SLC acknowledges financial support of University of LeicesterBrown Dwarfs are the coolest class of stellar objects known to date. Our present perception is
Ch Helling, Sarah L Casewell, Helling Christiane   +2 more
exaly   +2 more sources

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Ultracool Objects: L, T, and Y Dwarfs

2013
The discovery of the first bona fide brown dwarfs in 1995 ushered in a new era in both stellar and planetary astrophysics. The emergent spectra of brown dwarfs are distinct from those of the lowest-mass stars and thus the creation of three new spectral classes, L, T, and Y, were required in order to classify them.
openaire   +1 more source

Ultracool dwarfs observed with the Spitzer infrared spectrograph – II. Emergence and sedimentation of silicate clouds in L dwarfs, and analysis of the full M5–T9 field dwarf spectroscopic sample

Monthly Notices of the Royal Astronomical Society, 2022
Genaro Suarez, Stanimir Metchev
exaly  

3D spectroscopic analysis of helium-line white dwarfs

Monthly Notices of the Royal Astronomical Society, 2021
E Cukanovaite, P -E Tremblay, P Bergeron   +2 more
exaly  

The 40 pc sample of white dwarfs from Gaia

Monthly Notices of the Royal Astronomical Society, 2023
Mairi W O'Brien, D Koester, E Cukanovaite   +2 more
exaly  

Gaia white dwarfs within 40 pc II: the volume-limited Northern hemisphere sample

Monthly Notices of the Royal Astronomical Society, 2020
P -E Tremblay, N P Gentile Fusillo, M A Hollands   +2 more
exaly  

Horizontal spreading of planetary debris accreted by white dwarfs

Monthly Notices of the Royal Astronomical Society, 2021
Tim Cunningham, P -E Tremblay, Evan B Bauer   +2 more
exaly