Results 31 to 40 of about 30,446 (206)
X-ray extinction from interstellar dust [PDF]
Aims. We present a study on the prospects of observing carbon, sulfur, and other lower abundance elements (namely Al, Ca, Ti, and Ni) present in the interstellar medium using future X-ray instruments. We focus in particular on the detection and characterization of interstellar dust along the lines of sight. Methods.
Costantini, E. +5 more
openaire +3 more sources
Dust in the diffuse interstellar medium [PDF]
We present a model for the diffuse interstellar dust that explains the observed wavelength-dependence of extinction, emission, linear and circular polarisation of light. The model is set-up with a small number of parameters. It consists of a mixture of amorphous carbon and silicate grains with sizes from the molecular domain of 0.5 up to about 500nm ...
Siebenmorgen, R. +2 more
openaire +2 more sources
The Power of the Rings: The GRB 221009A Soft X-Ray Emission from Its Dust-scattering Halo
GRB 221009A is the brightest gamma-ray burst (GRB) ever detected that has occurred at low Galactic latitude. Owing to this exceptional combination, its prompt X-ray emission could be detected for weeks in the form of expanding X-ray rings produced by ...
Andrea Tiengo +13 more
doaj +1 more source
Constraints on interstellar dust models from extinction and spectro-polarimetry [PDF]
We present polarisation spectra of seven stars in the lines-of-sight towards the Sco OB1 association. Our spectra were obtained within the framework of the Large Interstellar Polarization Survey carried out with the FORS instrument of the ESO VLT. We have modelled the wavelength-dependence of extinction and linear polarisation with a dust model for the
Siebenmorgen, R. +3 more
openaire +2 more sources
Dust in the Small Magellanic Cloud: Interstellar Polarization and Extinction [PDF]
To elucidate the dust properties in the SMC we have for the first time measured linear polarization in five colors in the optical region of the spectrum for a sample of reddened stars. For two of these stars, for which there were no existing UV spectrophotometric measurements, but for which we measured a relatively large polarization, we have also ...
Rodrigues, C. V. +3 more
openaire +2 more sources
Estimating dust distances to Type Ia supernovae from colour excess time-evolution
We present a new technique to infer dust locations towards reddened Type Ia supernovae and to help discriminate between an interstellar and a circumstellar origin for the observed extinction. Using Monte Carlo simulations, we show that the time-evolution
Amanullah, R. +4 more
core +1 more source
VUV spectroscopy of carbon dust analogs: contribution to interstellar extinction [PDF]
10 pages, 10 figures, accepted to Astronomy & Astrophysics on 13/11 ...
Gavilan, L. +5 more
openaire +3 more sources
Interstellar extinction from photometric surveys: application to four high-latitude areas
Information on interstellar extinction and dust properties may be obtained from modern large photometric surveys data. Virtual Observatory facilities allow users to make a fast and correct cross-identification of objects from various surveys. It yields a
Malkov Oleg +13 more
doaj +1 more source
How dust absorbs and scatters starlight as a function of wavelength (known as the interstellar extinction curve) is crucial for correcting for the effects of dust extinction in inferring the true luminosity and colors of reddened astrophysical objects ...
Gao, Jian +3 more
core +1 more source
Life Cycle of Dust in the Magellanic Clouds and the Milky Way
To a great extent, our understanding of the life cycle of dust is based on the observational and theoretical studies of the Milky Way and the Magellanic Clouds, which will be the topic of this contribution. Over past years, a large volume of observations
Henning, Thomas, Zhukovska, Svitlana
core +1 more source

