Results 81 to 90 of about 17,929 (222)

Gas-phase Molecules in Protoplanetary Nebulae with the 21 μm Emission Feature

open access: yesThe Astronomical Journal
It has been more than 30 years since the enigmatic 21 μ m emission feature was first discovered in protoplanetary nebulae (PPNs). Although dozens of different dust carrier candidates have been proposed, there is as yet no widely accepted one.
Jian-Jie Qiu   +8 more
doaj   +1 more source

Circumstellar matter, with particular reference to jets and molecular flows [PDF]

open access: yesSymposium - International Astronomical Union, 1987
Circumstellar matter exists in many forms, such as winds from early and from late type stars, in infra-red sources and OH and H2O masers, in X-ray sources and jets, and molecular flows and Herbig-Haro objects. There is considerable diversity in the nature of the starlike bodies that underlie these phenomena.
openaire   +2 more sources

Electron microscopy observations of the diversity of Ryugu organic matter and its relationship to minerals at the micro‐ to nano‐scale

open access: yesMeteoritics &Planetary Science, Volume 59, Issue 8, Page 2023-2043, August 2024.
Abstract Transmission electron microscopy analyses of Hayabusa2 samples show that Ryugu organic matter exhibits a range of morphologies, elemental compositions, and carbon functional chemistries consistent with those of carbonaceous chondrites that have experienced low‐temperature aqueous alteration.
Rhonda M. Stroud   +112 more
wiley   +1 more source

Effect of Matter Accretion on Lithium Enhancement of Giants

open access: yesThe Astrophysical Journal
A subset of low-mass giants (
Xue-Feng Li   +5 more
doaj   +1 more source

Multi-dimensional models of circumstellar shells around evolved massive stars

open access: yes, 2012
Massive stars shape their surrounding medium through the force of their stellar winds, which collide with the circumstellar medium. Because the characteristics of these stellar winds vary over the course of the evolution of the star, the circumstellar ...
Keppens, Rony, van Marle, Allard Jan
core   +1 more source

The circumstellar disc in the Bok globule CB 26: Multi-wavelength observations and modelling of the dust disc and envelope [PDF]

open access: yes, 2009
Circumstellar discs are expected to be the nursery of planets. Grain growth within such discs is the first step in the planet formation process. The Bok globule CB 26 harbours such a young disc.
Alonso-Albi   +64 more
core   +4 more sources

Barotropic thin shells with linear EOS as models of stars and circumstellar shells in general relativity [PDF]

open access: yes, 1999
The spherically symmetric thin shells of the barotropic fluids with the linear equation of state are considered within the frameworks of general relativity.
Coleman S.   +4 more
core   +2 more sources

JWST imaging of the closest globular clusters—I. Possible infrared excess among white dwarfs in NGC 6397

open access: yesAstronomische Nachrichten, Volume 345, Issue 6-7, July-August 2024.
Abstract We present James Webb Space Telescope observations of the globular cluster NGC 6397 and use them to extend to infrared wavelengths the characterization of the cluster's entire white dwarf (WD) cooling sequence (CS). The data allows us to probe fundamental astrophysical WD properties and to search for evidence in their colors for (or against ...
L. R. Bedin   +11 more
wiley   +1 more source

SN 2022jox: An Extraordinarily Ordinary Type II SN with Flash Spectroscopy

open access: yesThe Astrophysical Journal
We present high-cadence optical and ultraviolet (UV) observations of the Type II supernova (SN), SN 2022jox which exhibits early spectroscopic high-ionization flash features of H i , He ii , C iv , and N iv that disappear within the first few days after ...
Jennifer E. Andrews   +22 more
doaj   +1 more source

On the Circumstellar Matter Distribution around Herbig Ae/Be Stars

open access: yesThe Astrophysical Journal, 1997
The spectral energy distributions (SEDs) observed in Herbig Ae/Be stars are critically analyzed in connection with a spherically symmetric model for matter distribution around the central objects. The possibility that the dusty component is described by an MRN-DL mixture (see the work of Mathis, Rumpl, and Nordsiek; Draine and Lee) and is constituted ...
PEZZUTO S.   +2 more
openaire   +2 more sources

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