Results 241 to 250 of about 8,365,552 (275)

Extended hot dust emission around the earliest massive quiescent galaxy

open access: yes
Ji Z   +16 more
europepmc   +1 more source

A Faint Progenitor System for the Faint Supernova 2024vjm

open access: yes
Zimmerman E   +69 more
europepmc   +1 more source

Satellites of Late-Type Spiral Galaxies

open access: yesEAS 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   +2 more
openaire   +2 more sources

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
openaire   +1 more source

Late-type galaxies observed with SAURON

2006
ABSTRACT 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
openaire   +1 more source

Ionizing the Diffuse Interstellar Medium in Late-Type Galaxies

Astrophysics and Space Science, 2001
We 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
openaire   +1 more source

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.
openaire   +1 more source

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