Zobrazeno 1 - 10
of 56
pro vyhledávání: '"D. S. Mathewson"'
Autor:
D. S. Mathewson, V. L. Ford
Publikováno v:
Examining the Big Bang and Diffuse Background Radiations ISBN: 9780792338154
Peculiar velocity measurements of 2500 southern spiral galaxies show large-scale flows in the direction of the Hydra-Centaurus clusters which fully participate in the flow themselves. The flow is not uniform over this region and seems to be associate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::500532b2d00ca6680d73aa2d25d86c6f
https://doi.org/10.1007/978-94-009-0145-2_18
https://doi.org/10.1007/978-94-009-0145-2_18
Autor:
V. L. Ford, D. S. Mathewson
Publikováno v:
The Astrophysical Journal Supplement Series. 107:97
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::515e475af1c3872f7591e788f7ac6243
https://doi.org/10.1086/192356
https://doi.org/10.1086/192356
Autor:
D. S. Mathewson, V. L. Ford
Publikováno v:
The Astrophysical Journal. 434:L39
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c19e5c222c3940ddc87dd855f29cac99
https://doi.org/10.1086/187569
https://doi.org/10.1086/187569
Publikováno v:
The Astrophysical Journal Supplement Series. 81:413
The data from photometric and spectroscopic observations of 1355 southern spiral galaxies are presented and used to determine their distances and peculiar velocities via the Tully-Fisher (TF) relation. Luminosity profiles are presented for the 1355 g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8e0d7305ae53457895c6528458058707
https://doi.org/10.1086/191700
https://doi.org/10.1086/191700
Publikováno v:
The Astrophysical Journal. 389:L5
The first results of a survey of the peculiar velocities of 1355 spiral galaxies in the southern sky using the Tully-Fisher relation to estimate their distances are presented. The most important result of these measurements is that no back-side infal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c29814d9785acf4ccf71794f800fec2
https://doi.org/10.1086/186335
https://doi.org/10.1086/186335
Publikováno v:
Highlights of Astronomy. 9:685-685
We have recently completed a survey of the peculiar velocities of 1355 southern spiral galaxies. The Tully – Fisher relation was used to estimate the distances to the spirals. The photometry was done in the I-band using CCDs on the lm telescope and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e59a150251b66ad53a1ac4c5b0b97bfb
https://doi.org/10.1017/s1539299600010042
https://doi.org/10.1017/s1539299600010042
Autor:
D. S. Mathewson
Publikováno v:
Australian Journal of Physics. 43:167
A brief review is made of the observational work on large-scale streaming motions in the Local Universe. There is considerable controversy as to whether the Great Attractor model of these streaming motions is correct. Preliminary results are presente
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8ce1656275965b620da99fdbd94a6cd2
https://doi.org/10.1071/ph900167
https://doi.org/10.1071/ph900167
Autor:
V. L. Ford, D. S. Mathewson
Publikováno v:
Symposium - International Astronomical Union. 108:125-136
The global distribution of HI in the Magellanic System is shown in Figure 1. The gas covers some 1500 square degrees of sky and has a mass of 1.8 × 109 M⊙. There are four main components: the LMC, the SMC, the inter-Cloud region and the Magellanic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7b61b06d69ad17458c14523b3ddecc7a
https://doi.org/10.1017/s0074180900040092
https://doi.org/10.1017/s0074180900040092
Publikováno v:
Symposium - International Astronomical Union. 101:559-565
We report the optical identification of four Balmer-dominated supernova remnants (SNRs) in the Large Magellanic Cloud. Both the Balmer-dominated spectra and the presence of a broad Hα component in one remnant can be understood in terms of a very hig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::392d2ba25cb891c314aae4e8ab708d07
https://doi.org/10.1017/s0074180900034434
https://doi.org/10.1017/s0074180900034434
Autor:
A. J. Kalnajs, H. Wehner, D. S. Mathewson, P. T. Rayner, J. B. Whiteoak, J. R. Forster, Richard N. Manchester, J. G. Ables, W. L. Peters
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 226:157-171
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e54dfbc376f82f7b0b164ffc01e5625
https://doi.org/10.1093/mnras/226.1.157
https://doi.org/10.1093/mnras/226.1.157