Results 251 to 260 of about 17,021 (292)

Evidence for a sub-Jovian planet in the young TWA 7 disk. [PDF]

Nature
Lagrange AM, Wilkinson C, Mâlin M, Boccaletti A, Perrot C, Matrà L, Combes F, Beust H, Rouan D, Chomez A, Milli J, Charnay B, Mazevet S, Flasseur O, Olofsson J, Bayo A, Kral Q, Carter A, Crotts KA, Delorme P, Chauvin G, Thebault P, Rubini P, Kiefer F, Radcliffe A, Mazoyer J, Bodrito T, Stasevic S, Langlois M.   +28 more
europepmc   +1 more source

Formation time-scales for stellar bars in diverse galactic discs. [PDF]

Mon Not R Astron Soc
Frosst M, Obreschkow D, Ludlow A.
europepmc   +1 more source

Are we there yet with XNA aptamers? [PDF]

RSC Adv
Chaillou S, Thonon S, Reynders S, Lescrinier E, Pinheiro VB.   +4 more
europepmc   +1 more source

<i>Atkinsonella hypoxylon</i> virus capsid structure highlights the diversity of capsid proteins among the <i>Partitiviridae</i>. [PDF]

J Gen Virol
Venturi M, Calthorpe-Byrne M, Aftret B, McNeale D, Rehm BHA, Sainsbury F.   +5 more
europepmc   +1 more source

Galaxy Tomography with the Gravitational Wave Background from Supermassive Black Hole Binaries

Chen Y.
europepmc   +1 more source

Galaxy And Mass Assembly (GAMA): the signatures of galaxy interactions as viewed from small-scale galaxy clustering [PDF]

Monthly Notices of the Royal Astronomical Society, 2018
Statistical studies of galaxy-galaxy interactions often utilise net change in physical properties of progenitors as a function of the separation between their nuclei to trace both the strength and the observable timescale of their interaction.
M L P Gunawardhana, Jon Loveday, A M Hopkins   +2 more
exaly   +3 more sources

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Galaxies in Interaction

Astronomische Nachrichten, 2004
AbstractPosters: Because of the large number of contributions, some oral presentations had to be transferred into Posters. The reader is referred to the final programme for the actual allocation of Posters.A01 Chemical Enrichment of the Intracluster MediumA02 Structural analysis of high‐velocity clouds – Evidence for an interaction between the Milky ...
Hüttemeister, Susanne, Zeilinger, Werner, Theis, Christian   +2 more
openaire   +1 more source

Galaxy And Mass Assembly (GAMA): the effect of close interactions on star formation in galaxies

Monthly Notices of the Royal Astronomical Society, 2015
The modification of star formation (SF) in galaxy interactions is a complex process, with SF observed to be both enhanced in major mergers and suppressed in minor pair interactions.
L J M Davies, A S G Robotham, Simon P Driver   +2 more
exaly   +3 more sources

Dynamics of Interacting Galaxies

Annual Review of Astronomy and Astrophysics, 1992
The dynamics of interacting galaxies as observed in the present epoch is reviewed. Topics discussed include numerical methods for modeling galactic interactions, the signatures of interacting galaxies due to tidal forces, and events that add mass to a galaxy.
Joshua E. Barnes, Lars Hernquist
openaire   +2 more sources

Galaxy Interactions and the Radio Galaxy Phenomenon

1990
We have been studying powerful radio galaxies (which we define as having radio power at 178MHz, P 178 ≥ 5xl024 Watts/Hz for a cosmology of H o = 100 km sec-1 Mpc-1 and q o = 0) in order to determine their origins. There are two distinct classes of powerful radio galaxies (PRGs), the so called class A and B radio galaxies (Hine and Longair 1979; Heckman
E. P. Smith, T. M. Heckman
openaire   +1 more source