Results 21 to 30 of about 10,749 (290)

Homogeneous Velocity‐Distance Data for Peculiar Velocity Analysis. III. The Mark III Catalog of Galaxy Peculiar Velocities [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 1997
This is the third in a series of papers in which we assemble and analyze a homogeneous catalog of peculiar velocity data. In Papers I and II, we described the Tully-Fisher (TF) redshift-distance samples that constitute the bulk of the catalog, and our methodology for obtaining mutually consistent TF calibrations for these samples.
Willick, Jeffrey A.   +5 more
openaire   +2 more sources

Cosmic string induced peculiar velocities [PDF]

open access: yesThe Astrophysical Journal, 1988
This paper considers the scenario of a flat universe with a network of heavy cosmic strings as the primordial fluctuation spectrum. The joint probability of finding streaming velocities of at least 600 km/s on large scales and local peculiar velocities of less than 800 km/s is calculated.
Anthony van Dalen, David N. Schramm
openaire   +3 more sources

Cosmology with peculiar velocities: observational effects [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2016
11 pages, 5 figures.
Andersen, P., Davis, T. M., Howlett, C.
openaire   +3 more sources

Peculiar velocities in dynamic spacetimes [PDF]

open access: yesPhysical Review D, 2014
We investigate the asymptotic behavior of peculiar velocities in certain physically significant time-dependent gravitational fields. Previous studies of the motion of free test particles have focused on the \emph{collapse scenario}, according to which a double-jet pattern with Lorentz factor $ \to \infty$ develops asymptotically along the direction of
Bini Donato, Mashhoon Bahram
openaire   +4 more sources

Peculiar Velocities of Nearby Galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2006
Over the last five years, enormous progress in accurate distance measurements for nearby galaxies has been attained. The Hubble Space Telescope allows us to estimate distances of about 7–10% accuracy using red giant branch (RGB) up to 8 Mpc. Now we have very accurate distances for more than 200 galaxies within ~6 Mpc.
D. Makarov   +9 more
openaire   +1 more source

The RMS Peculiar Velocity of Clusters [PDF]

open access: green, 1997
We study the rms peculiar velocity of clusters as a convenient statistic to put constraints on cosmological models. This statistic is easy to compute theoretically given a model for the power spectrum; we show that with some assumptions it can be directly related to the quantity $ _0^{0.6} _8$.
Richard Watkins
openalex   +3 more sources

Peculiar velocities and the mean density parameter [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1999
We study the peculiar velocity field inferred from the Mark III spirals using a new method of analysis. We estimate optimal values of Tully-Fisher scatter and zero-point offset, and we derive the 3-dimensional rms peculiar velocity ($ _v$) of the galaxies in the samples analysed.
Padilla, Nelson, Lambas, Diego G.
openaire   +2 more sources

Power spectrum shape from peculiar velocity data [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2007
10 pages, 2 figures, 3 tables, some changes to reflect published ...
Watkins, Richard, Feldman, Hume A.
openaire   +2 more sources

Transient hexagonal structures in sheared emulsions of isotropic inclusions on smectic bubbles in microgravity conditions

open access: yesScientific Reports, 2021
We describe the collective behavior of isotropic droplets dispersed over a spherical smectic bubble, observed under microgravity conditions on the International Space Station (ISS).
P. V. Dolganov   +8 more
doaj   +1 more source

A New Estimate of the Local Standard of Rest from Data on Young Objects

open access: yesOpen Astronomy, 2015
To estimate the peculiar velocity of the Sun with respect to the Local Standard of Rest (LSR), we use young objects in the Solar neighborhood with distance measurement errors within 10%–15%.
Bobylev V. V., Bajkova A. T.
doaj   +1 more source

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