Results 81 to 90 of about 17,929 (222)
Gas-phase Molecules in Protoplanetary Nebulae with the 21 μm Emission Feature
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]
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
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
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
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]
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]
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
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
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
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

