Matches in SemOpenAlex for { <https://semopenalex.org/work/W3105900570> ?p ?o ?g. }
- W3105900570 endingPage "305" @default.
- W3105900570 startingPage "277" @default.
- W3105900570 abstract "We present peculiar velocities for 85 clusters of galaxies in two large volumes at distances between 6000 and 15 000 km s−1 in the directions of Hercules-Corona Borealis and Perseus-Pisces-Cetus (the EFAR sample). These velocities are based on Fundamental Plane (FP) distance estimates for early-type galaxies in each cluster. We fit the FP using a maximum likelihood algorithm which accounts for both selection effects and measurement errors, and yields FP parameters with smaller bias and variance than other fitting procedures. We obtain a best-fitting FP with coefficients consistent with the best existing determinations. We measure the bulk motions of the sample volumes using the 50 clusters with the best-determined peculiar velocities. We find that the bulk motions in both regions are small, and consistent with zero at about the 5 per cent level. The EFAR results are in agreement with the small bulk motions found by Dale et al. on similar scales, but are inconsistent with pure dipole motions having the large amplitudes found by Lauer & Postman and Hudson et al. The alignment of the EFAR sample with the Lauer & Postman dipole produces a strong rejection of a large-amplitude bulk motion in that direction, but the rejection of the Hudson et al. result is less certain because their dipole lies at a large angle to the main axis of the EFAR sample. We employ a window function covariance analysis to make a detailed comparison of the EFAR peculiar velocities with the predictions of standard cosmological models. We find that the bulk motion of our sample is consistent with most cosmological models that approximately reproduce the shape and normalization of the observed galaxy power spectrum. We conclude that existing measurements of large-scale bulk motions provide no significant evidence against standard models for the formation of structure." @default.
- W3105900570 created "2020-11-23" @default.
- W3105900570 creator A5002739022 @default.
- W3105900570 creator A5014464961 @default.
- W3105900570 creator A5024884126 @default.
- W3105900570 creator A5057149667 @default.
- W3105900570 creator A5071141538 @default.
- W3105900570 creator A5074510228 @default.
- W3105900570 date "2001-02-21" @default.
- W3105900570 modified "2023-09-24" @default.
- W3105900570 title "The peculiar motions of early-type galaxies in two distant regions -- VII. Peculiar velocities and bulk motions" @default.
- W3105900570 cites W1555895019 @default.
- W3105900570 cites W1963537231 @default.
- W3105900570 cites W1970494468 @default.
- W3105900570 cites W1974328695 @default.
- W3105900570 cites W1976824203 @default.
- W3105900570 cites W1980118658 @default.
- W3105900570 cites W1980708053 @default.
- W3105900570 cites W1983651946 @default.
- W3105900570 cites W2003516208 @default.
- W3105900570 cites W2006497442 @default.
- W3105900570 cites W2007925985 @default.
- W3105900570 cites W2011802174 @default.
- W3105900570 cites W2019468284 @default.
- W3105900570 cites W2019511225 @default.
- W3105900570 cites W2019700971 @default.
- W3105900570 cites W2022527063 @default.
- W3105900570 cites W2025181530 @default.
- W3105900570 cites W2026792421 @default.
- W3105900570 cites W2037572085 @default.
- W3105900570 cites W2041611552 @default.
- W3105900570 cites W2042367512 @default.
- W3105900570 cites W2042905846 @default.
- W3105900570 cites W2045225546 @default.
- W3105900570 cites W2047862113 @default.
- W3105900570 cites W2052235912 @default.
- W3105900570 cites W2057363669 @default.
- W3105900570 cites W2059913799 @default.
- W3105900570 cites W2072925270 @default.
- W3105900570 cites W2103355920 @default.
- W3105900570 cites W2111817932 @default.
- W3105900570 cites W2123090155 @default.
- W3105900570 cites W2150681584 @default.
- W3105900570 cites W2156449290 @default.
- W3105900570 cites W2166814121 @default.
- W3105900570 cites W2603354544 @default.
- W3105900570 cites W2952179566 @default.
- W3105900570 cites W3099911513 @default.
- W3105900570 cites W3102188644 @default.
- W3105900570 cites W3103827746 @default.
- W3105900570 cites W3122756111 @default.
- W3105900570 cites W4253623486 @default.
- W3105900570 doi "https://doi.org/10.1046/j.1365-8711.2001.04044.x" @default.
- W3105900570 hasPublicationYear "2001" @default.
- W3105900570 type Work @default.
- W3105900570 sameAs 3105900570 @default.
- W3105900570 citedByCount "101" @default.
- W3105900570 countsByYear W31059005702012 @default.
- W3105900570 countsByYear W31059005702013 @default.
- W3105900570 countsByYear W31059005702014 @default.
- W3105900570 countsByYear W31059005702015 @default.
- W3105900570 countsByYear W31059005702016 @default.
- W3105900570 countsByYear W31059005702017 @default.
- W3105900570 countsByYear W31059005702018 @default.
- W3105900570 countsByYear W31059005702020 @default.
- W3105900570 countsByYear W31059005702021 @default.
- W3105900570 countsByYear W31059005702023 @default.
- W3105900570 crossrefType "journal-article" @default.
- W3105900570 hasAuthorship W3105900570A5002739022 @default.
- W3105900570 hasAuthorship W3105900570A5014464961 @default.
- W3105900570 hasAuthorship W3105900570A5024884126 @default.
- W3105900570 hasAuthorship W3105900570A5057149667 @default.
- W3105900570 hasAuthorship W3105900570A5071141538 @default.
- W3105900570 hasAuthorship W3105900570A5074510228 @default.
- W3105900570 hasBestOaLocation W31059005701 @default.
- W3105900570 hasConcept C106996143 @default.
- W3105900570 hasConcept C120665830 @default.
- W3105900570 hasConcept C121332964 @default.
- W3105900570 hasConcept C121955636 @default.
- W3105900570 hasConcept C144133560 @default.
- W3105900570 hasConcept C173523689 @default.
- W3105900570 hasConcept C174802034 @default.
- W3105900570 hasConcept C17825722 @default.
- W3105900570 hasConcept C180205008 @default.
- W3105900570 hasConcept C196083921 @default.
- W3105900570 hasConcept C198531522 @default.
- W3105900570 hasConcept C2524010 @default.
- W3105900570 hasConcept C2993021520 @default.
- W3105900570 hasConcept C33923547 @default.
- W3105900570 hasConcept C44870925 @default.
- W3105900570 hasConcept C62520636 @default.
- W3105900570 hasConcept C77538465 @default.
- W3105900570 hasConcept C97355855 @default.
- W3105900570 hasConcept C98444146 @default.
- W3105900570 hasConceptScore W3105900570C106996143 @default.
- W3105900570 hasConceptScore W3105900570C120665830 @default.
- W3105900570 hasConceptScore W3105900570C121332964 @default.
- W3105900570 hasConceptScore W3105900570C121955636 @default.