Results 241 to 250 of about 8,365,552 (275)
Extended hot dust emission around the earliest massive quiescent galaxy
Ji Z +16 more
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A detailed analysis of the Czernik 38 cluster and its associated tidal tail, utilizing Gaia DR3 and 2MASS. [PDF]
Ahmed NM.
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Perspectives on the physics of late-type stars from beyond low earth orbit, the moon and mars. [PDF]
Mathur S, Santos ÂRG.
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A Faint Progenitor System for the Faint Supernova 2024vjm
Zimmerman E +69 more
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Satellites of Late-Type Spiral Galaxies
Using VIMOS (VLT) we carried out a spectroscopic survey around seven late-type spiral galaxies and we discovered 55 satellites. After obtaining the radial velocities and spatial distribution of the satellites, we analyze their properties.
I. A. Yegorova +2 more
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Anomalous dust in late-type galaxies
EAS Publications Series, 2011The last quarter century has seen a tremendous increase in quantitative information on the dust in galaxies. Yet, essential knowledge is still lacking. Recent results underline how determinations of dust mass and dust-to-gas ratio in galaxies are still beset by very considerable uncertainties.
F.P. Israel, C. Bot
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Late-type galaxies observed with SAURON
2006ABSTRACT We present the stellar and gas kinematics of a sample of 18 nearby late-type spiral galaxies (Hubble types ranging from Sb to Sd), observed with the integral-field spectrograph SAURON at the 4.2-m William Herschel Telescope. SAURON covers the spectral range 4800-5380 Å, allowing us to measure the Hβ, Fe, Mgb absorption features and the ...
Ganda, Katia +7 more
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Ionizing the Diffuse Interstellar Medium in Late-Type Galaxies
Astrophysics and Space Science, 2001We show how the clumpy structure of the interstellar medium (ISM) both inside HII regions and in the diffuse component, permits the propagation of ionizing photons from OB stars on kiloparsec scales.
J.E. Beckman, A. Zurita, M. Rozas
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Cold Gas in Late-Type Galaxies
1992In the last two decades a large number of spiral galaxies have been studied in the 21-cm line. These studies have revealed the density distribution and kinematics of HI and have provided the measurements of the total mass and the mass distribution in those systems.
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