Zobrazeno 1 - 10
of 209
pro vyhledávání: '"URSA-MAJOR CLUSTER"'
Akademický článek
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Autor:
Ximena Fernández, J. H. van Gorkom, N. Luber, Kevin Vinsen, Attila Popping, Richard Dodson, J. M. van der Hulst, Julie D. Davis, Emmanuel Momjian, Daniel J. Pisano, Kelley M. Hess, M. S. Yun, J. Blue Bird, Hansung B. Gim, Kathryn Kreckel, A. Chung, Eric M. Wilcots, D. M. Lucero
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 492(1), 153-176. Oxford University Press
We present neutral hydrogen (HI) and ionized hydrogen (H${\alpha}$) observations of ten galaxies out to a redshift of 0.1. The HI observations are from the first epoch (178 hours) of the COSMOS HI Large Extragalactic Survey (CHILES). Our sample is HI
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed42f0ee84ee140d5675a8f5e2d2324b
https://research.rug.nl/en/publications/e476bb54-bc22-4a1d-91cf-37ba818050cb
https://research.rug.nl/en/publications/e476bb54-bc22-4a1d-91cf-37ba818050cb
Akademický článek
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Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 469 (2), pp.2387-2400. ⟨10.1093/mnras/stx1018⟩
Monthly Notices of the Royal Astronomical Society, 2017, 469 (2), pp.2387-2400. ⟨10.1093/mnras/stx1018⟩
Monthly Notices of the Royal Astronomical Society, 469(2), 2387-2400. Oxford University Press
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 469 (2), pp.2387-2400. ⟨10.1093/mnras/stx1018⟩
Monthly Notices of the Royal Astronomical Society, 2017, 469 (2), pp.2387-2400. ⟨10.1093/mnras/stx1018⟩
Monthly Notices of the Royal Astronomical Society, 469(2), 2387-2400. Oxford University Press
In this paper we investigate the statistical properties of the Tully-Fisher relation for a sample of 32 galaxies with measured distances from the Cepheid period-luminosity relation and/or TRGB stars. We take advantage of panchromatic photometry in 12
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ffebc9a483236cf81c533135924ad7c3
https://ora.ox.ac.uk/objects/uuid:41cdc8ee-9226-471f-a64d-a362945e1efd
https://ora.ox.ac.uk/objects/uuid:41cdc8ee-9226-471f-a64d-a362945e1efd
We present our results of the spectroscopic study of the lenticular galaxy NGC 4143 - an outskirt member of the Ursa Major cluster. Using the observations at the 6-m SAO RAS telescope with the SCORPIO-2 spectrograph and also the archive data of panor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::36b6dc49285092e32fe2d3fdb847ce37
Publikováno v:
Universitas Scientiarum, Vol 23, Iss 2, Pp 191-218 (2018)
Maximum disc mass models for a set of spiral galaxies from the Ursa Major Cluster are presented. We construct the models using the Hunther method and the particular solutions are chosen in such away that the circular velocities are adjusted very accu
Publikováno v:
Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales, Volume: 43, Issue: 166, Pages: 24-30, Published: MAR 2019
Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales
Revista de la Academia Colombiana de Ciencias Exactas, Físicas y Naturales
In the present paper, using a generalization of the Miyamoto and Nagai potential we adjusted the observed rotation curves of three specific spiral galaxies to the analytical circular velocities. The observational data have been taken from a 21 cm-lin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a25a90d15aba3734790263b62e53b576
http://arxiv.org/abs/1907.09573
http://arxiv.org/abs/1907.09573
Autor:
Filippo Fraternali, Justin I. Read, Giuliano Iorio, Carlo Nipoti, Giuseppina Battaglia, Enrico M. Di Teodoro
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 466(4), 4159-4192. Oxford University Press
Dwarf Irregular galaxies (dIrrs) are the smallest stellar systems with extended HI discs. The study of the kinematics of such discs is a powerful tool to estimate the total matter distribution at these very small scales. In this work, we study the HI
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eaa476cd5dcfdcab134ad56cabe259d9
https://research.rug.nl/en/publications/1073e20b-5a7f-4ac1-8716-6f188bb9d7be
https://research.rug.nl/en/publications/1073e20b-5a7f-4ac1-8716-6f188bb9d7be
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 463(4), 4052-4067. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2016, 463, pp.4052-4067. ⟨10.1093/mnras/stw2213⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2016, 463, pp.4052-4067. ⟨10.1093/mnras/stw2213⟩
We present spatially-resolved HI kinematics of 32 spiral galaxies which have Cepheid or/and Tip of the Red Giant Branch distances, and define a calibrator sample for the Tully-Fisher relation. The interferometric HI data for this sample were collecte
Akademický článek
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