Results 111 to 120 of about 25,802 (223)

Observational constraints on circumstellar dust [PDF]

open access: yes
There is an enormous range in the properties of stars that are losing mass. The red giants responsible for injecting roughly half or more of the material into the interstellar medium are reviewed. The physical properties are described for the out flowing
Jura, M.
core   +1 more source

Spinning Dust Emission from Circumstellar Disks and Its Role In Excess Microwave Emission [PDF]

open access: bronze, 2018
Thiem Hoang   +3 more
openalex   +1 more source

The Presolar Grain Database. I. Silicon Carbide

open access: yesThe Astrophysical Journal Supplement Series
The Presolar Grain Database (PGD) contains the vast majority of isotope data (published and unpublished) on presolar grains and was first released as a collection of spreadsheets in 2009.
Thomas Stephan   +10 more
doaj   +1 more source

Radiation-driven acceleration in the expanding WR140 dust shell. [PDF]

open access: yesNature, 2022
Han Y, Tuthill PG, Lau RM, Soulain A.
europepmc   +1 more source

Correlated Molybdenum, Ruthenium, and Barium Isotope Anomalies in Presolar Silicon Carbide Grains

open access: yesThe Astrophysical Journal
We have analyzed molybdenum, ruthenium, and barium isotopes simultaneously in 55 individual presolar silicon carbide (SiC) grains from the Murchison CM2 meteorite using the Chicago Instrument for Laser Ionization (or CHILI).
Thomas Stephan   +5 more
doaj   +1 more source

Discovery of a Variable Yellow Supergiant Progenitor for the Type IIb SN 2024abfo

open access: yesThe Astrophysical Journal Letters
We report the discovery of a progenitor candidate for the Type IIb SN 2024abfo using multiepoch pre-explosion images from the Hubble Space Telescope and the Dark Energy Camera Legacy Survey.
Zexi Niu   +6 more
doaj   +1 more source

Intermediate-Mass Mergers: A New Scenario for Several FS CMa Stars

open access: yesGalaxies
We summarise the properties and nature of a peculiar group of B-type stars called FS CMa stars. These stars show the B[e] phenomenon, i.e., their spectra exhibit both forbidden emission lines and infrared excess.
Daniela Korčáková   +8 more
doaj   +1 more source

History of two mass loss processes in VY CMa. [PDF]

open access: yesProc Int Astron Union, 2023
Quintana-Lacaci G   +6 more
europepmc   +1 more source

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