Results 111 to 120 of about 19,928 (198)
Studies of interstellar reddening
The wavelength dependence of interstellar obscuration, in magnitudes against reciprocal wavelength, is known to be well represented, over the visible part of the spectrum, by two straight lines intersecting at or near the broad interstellar absorption band at 4430A. The existing measures, obtained principally from low dispersion objective prism spectra,
openaire +1 more source
Diffuse interstellar bands in the near-infrared: expanding the reddening range
ABSTRACT We have investigated the behaviour of three strong near-infrared diffuse interstellar bands (DIBs) at λ13177 Å, λ14680 Å, and λ15272 Å, on a larger sample of sightlines and over a wider range of extinctions than previously studied, utilizing spectra from three observatories.
R Castellanos +4 more
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Recent observations have revealed that dust is widespread and abundant in galaxies up to z ≃ 8, significantly influencing their appearance and spectral properties.
He Zhao, Bingqiu Chen, Jun Li
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Considering light-matter interactions in the Friedmann equations. [PDF]
Vavryčuk V.
europepmc +1 more source
A Survey of Recent Interstellar Reddening Observations [PDF]
K. Nandy, N. C. Wickramasinghe
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Photographic Photometry of NGC 6866
. Magnitudes and colors in the UBV photometric system have been determined for 575 stars in and around NGC 6866. The color-color relation of the cluster stars provides an estimate of interstellar reddening of 0.16 mag. The distance of cluster is found to
B. Hidajat, W. Sutantyo
doaj
Connecting Dust and Outflows in Active Galactic Nuclei: The Intriguing Case of NGC 6860
Cosmic dust plays a crucial role in the evolution of galaxies, significantly influencing star formation and the interstellar medium. However, in active galactic nuclei (AGNs), the role and origin of dust remain poorly understood.
I. Psaradaki +6 more
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Interstellar reddening in the galaxy
Objective prism spectra obtained with the 16/24/60-inch Schmidt telescope have been used for an investigation of the wavelength dependence of interstellar absorption in the spectral range from 8000A to 3450A, in a region of 30 square degrees in Cygnus centred on (20ʰ15ᵐ, 38 °).
openaire +1 more source
A radio-detected type Ia supernova with helium-rich circumstellar material. [PDF]
Kool EC +36 more
europepmc +1 more source
Planetary nebulae (PNe) shown to be members of star clusters provide information on their properties and evolutionary histories that cannot be determined for PNe in the field, in particular the initial masses of their progenitor stars.
Andrea Bellini +2 more
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