Results 11 to 20 of about 1,775 (210)

From tidal dwarf galaxies to satellite galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2006
Accepted for publication in A&A. Shortened abstract below, full version in the paper.
Bournaud, Frédéric, Duc, Pierre-Alain
openaire   +4 more sources

Dynamical Friction on Satellite Galaxies [PDF]

open access: yesPublications of the Astronomical Society of Japan, 2006
Abstract For a rigid model satellite, Chandrasekhar’s dynamical friction formula describes the orbital evolution quite accurately, when the Coulomb logarithm is chosen appropriately. However, it is not known if the orbital evolution of a real satellite with the internal degree of freedom can be described by the dynamical friction formula.
Fujii, Michiko   +2 more
openaire   +2 more sources

Satellites and haloes of dwarf galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2012
We study the abundance of satellite galaxies as a function of primary stellar mass using the SDSS/DR7 spectroscopic catalogue. In contrast with previous studies, which focussed mainly on bright primaries, our central galaxies span a wide range of stellar mass, 10^7.5 < M_*^pri/M_sun < 10^11, from dwarfs to central cluster galaxies.
Sales, L.V.   +3 more
openaire   +4 more sources

A Census of Dwarf Galaxy Satellites around LMC-mass Galaxy NGC 2403

open access: yesThe Astrophysical Journal
We present the first comprehensive census of the satellite population around a Large Magellanic Cloud stellar-mass galaxy, as part of the Magellanic Analog Dwarf Companions and Stellar Halos (MADCASH) survey. We have surveyed NGC 2403 ( D = 3.0 Mpc) with
Jeffrey L. Carlin   +13 more
doaj   +4 more sources

THE LOPSIDED DISTRIBUTION OF SATELLITE GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2016
ABSTRACT The distribution of smaller satellite galaxies around large central galaxies has attracted attention because peculiar spatial and kinematic configurations have been detected in some systems. A particularly striking example of such behavior is seen in the satellite system of the Andromeda galaxy, where around 80% are on the near ...
Noam I. Libeskind   +3 more
openaire   +3 more sources

Retracted: Can the chemical industry solve the climate change?On the role of human energy production, renewable energies, and the potential of chemistry as a solution provider

open access: yesChemie Ingenieur Technik, EarlyView., 2023
Let us consider an alternative perspective on climate change: The sum of solar radiation and heat generated by human activity result in a net energy input of 1.96 times that of the Sun on the Earth's surface. The expanding global population is expected to exacerbate this issue. Potential solutions are proposed, including replacement and heat recycling.
Martin Bertau, Gerald Steiner
wiley   +1 more source

The anisotropic distribution of satellite galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2008
27 pages. Accepted for publication in MNRAS.
Bailin, Jeremy   +4 more
openaire   +5 more sources

Probing satellite quenching with galaxy clustering [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
Satellites within simulated massive clusters are significantly spatially correlated with each other, even when those satellites are not gravitationally bound to each other. This correlation is produced by satellites that entered their hosts relatively recently, and is undetectable for satellites that have resided in their hosts for multiple dynamical ...
Chamberlain, Robert T.   +3 more
openaire   +2 more sources

What determines satellite galaxy disruption? [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2010
19 pages, 14 figures, accepted for publication in ...
Andrew R. Wetzel, Martin White
openaire   +3 more sources

DWARF GALAXY CLUSTERING AND MISSING SATELLITES [PDF]

open access: yesThe Astrophysical Journal, 2009
At redshifts around 0.1 the CFHT Legacy Survey Deep fields contain some 6x10^4 galaxies spanning the mass range from 10^5 to 10^12 Msun. We measure the stellar mass dependence of the two point correlation using angular measurements to largely bypass the errors, approximately 0.02 in the median, of the photometric redshifts. Inverting the power-law fits
Carlberg, R. G.   +2 more
openaire   +2 more sources

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