Results 251 to 260 of about 553,808 (287)

Extended hot dust emission around the earliest massive quiescent galaxy

Ji Z, Williams C, Rieke G, Lyu J, Alberts S, Sun F, Helton J, Rieke M, Shivaei I, D'Eugenio F, Tacchella S, Robertson B, Zhu Y, Maiolino R, Bunker A, Sun Y, Willmer C.   +16 more
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Anti-TIGIT therapies: a review of preclinical and clinical efficacy and mechanisms. [PDF]

Cancer Immunol Immunother
Sundstrom EC, Huang X, Wiemer AJ.
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A Preliminary Luminosity Clssification of Late-Type Galaxies.

The Astrophysical Journal, 1960
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The photometry and kinematics studies of NGC 2509 derived from Gaia DR3. [PDF]

Sci Rep
Ahmed NM, Tadross AL.
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Modes of the Dark Ages 21 cm field accessible to a lunar radio interferometer. [PDF]

Philos Trans A Math Phys Eng Sci
Bull P, Guandalin C, Addis C.
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A binary merger product as the direct progenitor of a Type II-P supernova

Niu* Z, Sun* N, Zapartas* E, Souropanis D, Cui Y, Maund JR, Andrews JJ, Briel MM, Fraser M, Gossage S, Kruckow MU, Liotine C, Liu Z, Srivas PM, Teng E, Wang X, Yang Y, Liu J.   +17 more
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Satellites of Late-Type Spiral Galaxies

EAS Publications Series, 2011
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, PIZZELLA, ALESSANDRO, P. Salucci   +2 more
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Anomalous dust in late-type galaxies

EAS Publications Series, 2011
The 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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Cold Gas in Late-Type Galaxies

1992
In 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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Gaseous Halos of Late-Type Spiral Galaxies

Publications of the Astronomical Society of the Pacific, 1997
This article reviews the most recent observational results on disk-halo interactions in nearby galaxies. The implications of these results on our understanding of the structure of the interstellar medium (ISM) in our Galaxy and external spiral galaxies, with particular emphasis on the halo ISM, are discussed. Disk-halo interactions occur only above the
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