Results 31 to 40 of about 5,942,265 (309)

Evidence for Ultra-diffuse Galaxy “Formation” through Galaxy Interactions [PDF]

open access: yesThe Astrophysical Journal Letters, 2018
Abstract We report the discovery of two ultra-diffuse galaxies (UDGs) that show clear evidence of an association with tidal material and an interaction with a larger galaxy halo, found during a search of the Wide portion of the Canada–France–Hawaii Telescope Legacy Survey. The two new UDGs, NGC 2708-Dw1 and NGC 5631-Dw1, are faint (M
P. Bennet   +5 more
openaire   +2 more sources

SIDM on FIRE: hydrodynamical self-interacting dark matter simulations of low-mass dwarf galaxies. [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2017
We compare a suite of four simulated dwarf galaxies formed in 1010 M☉ haloes of collisionless cold dark matter (CDM) with galaxies simulated in the same haloes with an identical galaxy formation model but a non-zero cross-section for DM self-interactions.
V. Robles   +9 more
semanticscholar   +1 more source

PKS2250-41 and the Role of Jet Cloud Interactions in Powerful Radio Galaxies [PDF]

open access: yes, 1998
We have studied the effects of the interaction between the radio jet and the ambient gas in the powerful radio galaxy PKS2250-41 (z = 0.31). Our results show that the gas has been accelerated, compressed, heated and collisionally ionized by the shock ...
M. Villar-Martin   +10 more
semanticscholar   +1 more source

Prevalence of Tidal Interactions among Local Seyfert Galaxies: The Control Experiment [PDF]

open access: yes, 2008
We test whether there is a relation between the observed tidal interactions and Seyfert activity by imaging in atomic hydrogen (H I 27) inactive galaxies at the same spatial resolution and detection threshold as the Seyfert sample. This control sample of
Ya-wen Tang, C. Kuo, Jeremy Lim, P. Ho
semanticscholar   +1 more source

The evidence for jet-cloud interactions in a sample of high-redshift radio galaxies [PDF]

open access: yes, 2001
We present detailed long-slit spectroscopic observations of a sample of four powerful radio galaxies, with high redshifts (0 ...
C. Solórzano-Iñarrea   +4 more
semanticscholar   +1 more source

Reignition of star formation in dwarf galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
The Local Group hosts a number of star-forming dwarf galaxies that show evidence of periods of little to no star formation. We use a suite of cosmological simulations to study how star formation is reignited in such galaxies.
A. Wright   +3 more
semanticscholar   +1 more source

Scale Interactions and Galaxy Evolution [PDF]

open access: yesAstrophysics and Space Science, 2003
To understand galaxies and their evolution, it is necessary to describe how the different scales interact: how the microscopic physics, such as star formation, or the large scale physics, such as galaxy interactions may modify the galaxy global shapes.
openaire   +2 more sources

The large-scale distribution of warm ionized gas around nearby radio galaxies with jet-cloud interactions [PDF]

open access: yes, 2000
Deep, narrow-band Hα observations taken with the TAURUS Tunable Filter on the 4.2-m William Herschel Telescope are presented for two nearby radio galaxies with strong jet–cloud interactions.
C. Tadhunter   +5 more
semanticscholar   +1 more source

Triazine‐Trione Thermosets with High Processability for Scaffold Applications in Bone Tissue Engineering

open access: yesAdvanced Healthcare Materials, EarlyView.
Novel photo‐clickable triazine‐trione thermosets can be shaped and cured under mild conditions, including room and physiological temperatures. These materials are biocompatible and support osteogenic differentiation of bone marrow–derived mesenchymal stem cells on their surface.
Åshild Johansen   +7 more
wiley   +1 more source

Bar-spheroid interaction in galaxies

open access: yesThe Astrophysical Journal, 1992
The secular evolution of barred galaxies is explored using N-body simulation and linear analysis. In particular, we examine the interaction between bars and spheroidal components of galaxies. According to our calculations, this interaction drives secular transfer of angular momentum from bars to spheroids, primarily through resonant coupling.
Hernquist, Lars, Weinberg, Martin D.
openaire   +2 more sources

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