Results 31 to 40 of about 1,216,320 (294)
Direct imaging of molten protoplanets in nearby young stellar associations [PDF]
During their formation and early evolution, rocky planets undergo multiple global melting events due to accretionary collisions with other protoplanets.
Bower, Daniel J. +14 more
core +3 more sources
OB associations and their origins [PDF]
OB associations are unbound groups of young stars made prominent by their bright OB members, and have long been thought to be the expanded remnants of dense star clusters.
Wright
core +1 more source
A DETECTION OF GAS ASSOCIATED WITH THE M31 STELLAR STREAM [PDF]
10 pages, 5 figures, accepted for publication in the Astrophysical ...
Koch, Andreas +4 more
openaire +2 more sources
A stellar overdensity associated with the Small Magellanic Cloud [PDF]
14 pages, 10 color ...
Pieres, A. +67 more
openaire +7 more sources
cx2204/stellar-radius: stellar radius microphysics
Full Changelog: https://github.com/cx2204/stellar-radius/commits/v1.
cx2204
core +1 more source
ABSTRACT Pediatric gastroenteropancreatic neuroendocrine neoplasms (GEP‐NENs) are extremely rare and clinically heterogeneous. Management has largely been extrapolated from adult practice. This European Standard Clinical Practice Guideline (ESCP), developed by the EXPeRT network in collaboration with adult NEN experts, provides (adult) evidence ...
Michaela Kuhlen +23 more
wiley +1 more source
Kinematic Age of the β-Pictoris Moving Group
Accurate age estimation of nearby young moving groups (NYMGs) is important as they serve as crucial testbeds in various fields of astrophysics, including the formation and evolution of stars and planets, as well as loose stellar associations.
Jinhee Lee, Inseok Song
doaj +1 more source
Solid Pseudopapillary Neoplasm of the Pancreas in Children and Adolescents: Expert Recommendations
ABSTRACT Solid pseudopapillary neoplasm of the pancreas (SPN) is a rare low‐grade malignant exocrine pancreatic tumor, mostly discovered during the second decade of life in females, with a very good prognosis, provided microscopically complete surgical excision is achieved.
Sabine Irtan +18 more
wiley +1 more source
Kinematic Ages of the Tucana–Horologium, Columba, and Carina Associations
The traceback method allows the computation of the kinematic age of nearby young associations from astrometric and kinematic data alone, circumventing the need for stellar evolution models.
Dominic Couture +2 more
doaj +1 more source
A Census of the Circumstellar Disk Populations in the Sco-Cen Complex
I have used mid-infrared (IR) photometry from the Wide-field Infrared Survey Explorer (WISE) to perform a census of circumstellar disks among ∼10,000 candidate members of the Sco-Cen complex that were recently identified with data from the Gaia mission ...
K. L. Luhman
doaj +1 more source

