Zobrazeno 1 - 10
of 52
pro vyhledávání: '"R B Tully"'
The dwarf irregular galaxy HIPASS J1131-31 was discovered as a source of HI emission at low redshift in such close proximity of a bright star that we call it Peekaboo. The galaxy resolves into stars in images with Hubble Space Telescope, leading to a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a91237757c865e8e7fdeaa0db383935
We report observations of five dwarf galaxies in the vicinity of the luminous S0 galaxy NGC 3115 performed with the Advanced Camera for Surveys on the Hubble Space Telescope. Their distances determined via the Tip of the Red Giant Branch are: 10.05 M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2492905f47ffa68e938ed76593c849b9
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A113. ⟨10.1051/0004-6361/202039025⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A113. ⟨10.1051/0004-6361/202039025⟩
In this study, we present an update of a compilation of line width measurements of neutral atomic hydrogen (HI) galaxy spectra at 21 cm wavelength. Our All Digital HI (ADHI) catalog consists of the previous release augmented with our new HI observati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25a4b15566dbbde13f48e39d0e5ae392
https://hal.archives-ouvertes.fr/hal-03143631/document
https://hal.archives-ouvertes.fr/hal-03143631/document
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 501, 2608-2626. Oxford University Press
We determined the HI mass function of galaxies in the Ursa Major association of galaxies using a blind VLA-D array survey, consisting of 54 pointings in a cross pattern, covering the centre as well as the outskirts of the Ursa Major volume. The calcu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1e5092998cbd865fc0e5408f37452a2b
http://arxiv.org/abs/2012.03648
http://arxiv.org/abs/2012.03648
Autor:
Daniel Pomarède, Oliver Müller, Marcel S. Pawlowski, Hélène M. Courtois, Matthias Steinmetz, Alexander Knebe, Stefan Gottlöber, Jenny G. Sorce, Edoardo Carlesi, Noam I. Libeskind, R. B. Tully, Yehuda Hoffman
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 490 (3), pp.3786-3792. ⟨10.1093/mnras/stz2852⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 490 (3), pp.3786-3792. ⟨10.1093/mnras/stz2852⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 490 (3), pp.3786-3792. ⟨10.1093/mnras/stz2852⟩
Monthly Notices of the Royal Astronomical Society, 2019, 490 (3), pp.3786-3792. ⟨10.1093/mnras/stz2852⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 490 (3), pp.3786-3792. ⟨10.1093/mnras/stz2852⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 490 (3), pp.3786-3792. ⟨10.1093/mnras/stz2852⟩
To date at least 10 highly flattened planes of dwarf galaxies are claimed to have been discovered in the Local Universe. The origin of these planes of galaxies remains unknown. One suggestion is that they are related to the large-scale structure of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0c022873c68147c1c4108b9ca7ed654b
https://hal.science/hal-02431414
https://hal.science/hal-02431414
Autor:
Hélène M. Courtois, Yehuda Hoffman, Romain Graziani, Guilhem Lavaux, Y. Copin, Daniel Pomarède, R. B. Tully
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, 2019, 488 (4), pp.5438-5451. ⟨10.1093/mnras/stz078⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 488 (4), pp.5438-5451. ⟨10.1093/mnras/stz078⟩
Monthly Notices of the Royal Astronomical Society, 2019, 488 (4), pp.5438-5451. ⟨10.1093/mnras/stz078⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 488 (4), pp.5438-5451. ⟨10.1093/mnras/stz078⟩
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2019, 488 (4), pp.5438-5451. ⟨10.1093/mnras/stz078⟩
Monthly Notices of the Royal Astronomical Society, 2019, 488 (4), pp.5438-5451. ⟨10.1093/mnras/stz078⟩
A hierarchical Bayesian model is applied to the Cosmicflows-3 catalog of galaxy distances in order to derive the peculiar velocity field and distribution of matter within $z \sim 0.054$. The model assumes the $\Lambda$CDM model within the linear regi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f669f27d26e5ddcbe2a3809f569888da
https://hal.archives-ouvertes.fr/hal-01990691/document
https://hal.archives-ouvertes.fr/hal-01990691/document
Autor:
Jayaram N. Chengalur, Ayesha Begum, Luca Rizzi, Igor D. Karachentsev, Margarita Sharina, R. B. Tully, Lidia Makarova
Publikováno v:
Astronomische Nachrichten. 337:306-314
Observations are presented of the isolated dwarf irregular galaxy And IV made with the Hubble Space Telescope Advanced Camera for Surveys and the Giant Metrewave Radio Telescope in the 21 cm HI line. We determine the galaxy distance of 7.17 ± 0.31 M
Autor:
Igor D. Karachentsev, R. B. Tully, Edward J. Shaya, V. E. Karachentseva, L. N. Makarova, Luca Rizzi
We report HST/ACS observations of two nearby gas-rich dwarf galaxies: DDO 161 and UGCA 319. Their distances determined via the Tip of the Red Giant Branch are 6.03 (-0.21/+0.29) Mpc and 5.75+-0.18 Mpc, respectively. The galaxies form an isolated pair
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06d353c5e21a4ccbb067a146f377c81d
http://arxiv.org/abs/1704.07648
http://arxiv.org/abs/1704.07648
A faint dwarf irregular galaxy has been discovered in the HST/ACS field of LV J1157+5638. The galaxy is resolved into individual stars, including the brightest magnitude of the red giant branch. The dwarf is very likely a physical satellite of LV J11
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b72fb4aebeaae3502d75e17733f9fa0
Autor:
R. B. Tully, Hélène M. Courtois
Publikováno v:
Astronomische Nachrichten. 333:436-440
‘Cosmic Flows’ is a program to determine galaxy distances for 30000 galaxies with systematic errors below 2%, almost ten times the number currently known and a five-fold improvement in systematics. The resultant velocity field will provide input