Zobrazeno 1 - 10
of 82
pro vyhledávání: '"NGC 185"'
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 25, Iss 3, Pp 245-248 (2008)
We determined values of distance modulus to nearby dwarf galaxy NGC 185 from the Tip of Red-Giant Branch (TRGB) method. Apparent magnitudes of the TRGB are estimated from the near-infrared JHK luminosity functions (LFs) of the resolved giant branch s
Externí odkaz:
https://doaj.org/article/cb123f6f9a624b5c872b7747cb340ee5
Autor:
Nuwanthika Fernando, Annette M. N. Ferguson, Nicolas F. Martin, Rodrigo A. Ibata, Anthony R. Conn, Nicholas F. Bate, Geraint F. Lewis, Alan W. McConnachie, Veronica Arias, Magda Guglielmo, Joss Bland-Hawthorn, Mike Irwin
Publikováno v:
Arias, V, Guglielmo, M, Fernando, N, Lewis, G F, Bland-Hawthorn, J, Bate, N F, Conn, A, Irwin, M J, Ferguson, A M N, Ibata, R A, McConnachie, A W & Martin, N 2016, ' NGC 147, NGC 185 and CassII: a genetic approach to orbital properties, star formation and tidal debris ', Monthly Notices of the Royal Astronomical Society, vol. 456, no. 2, pp. 1654-1665 . https://doi.org/10.1093/mnras/stv2781
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 456 (2), pp.1654-1665. ⟨10.1093/mnras/stv2781⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 456 (2), pp.1654-1665. ⟨10.1093/mnras/stv2781⟩
NGC147, NGC185 and CassiopeiaII (CassII) have similar positions in the sky, distances and measured line of sight velocities. This proximity in phase space suggests that these three satellites of M31 form a subgroup within the Local Group. Nevertheles
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Lisa M. Young, Gianfranco Gentile, Diane Cormier, George J. Bendo, Robert C. Kennicutt, Matthew Smith, Maarten Baes, Médéric Boquien, Suzanne C. Madden, Jacopo Fritz, Ilse De Looze
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
De Looze, I, Baes, M, Bendo, G J, Fritz, J, Boquien, M, Cormier, D, Gentile, G, Kennicutt, R C, Madden, S C, Smith, M W L & Young, L 2016, ' The interstellar medium in Andromeda's dwarf spheroidal galaxies-I. Content and origin of the interstellar dust ', Monthly Notices of the Royal Astronomical Society, vol. 459, no. 4, pp. 3900-3916 . https://doi.org/10.1093/mnras/stw868
De Looze, I, Baes, M, Bendo, G J, Fritz, J, Boquien, M, Cormier, D, Gentile, G, Kennicutt, R C, Madden, S C, Smith, M W L & Young, L 2016, ' The interstellar medium in Andromeda's dwarf spheroidal galaxies-I. Content and origin of the interstellar dust ', Monthly Notices of the Royal Astronomical Society, vol. 459, no. 4, pp. 3900-3916 . https://doi.org/10.1093/mnras/stw868
Dwarf spheroidal galaxies are among the most numerous galaxy population in the Universe, but their main formation and evolution channels are still not well understood. The three dwarf spheroidal satellites (NGC147, NGC185, and NGC205) of the Andromed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6278dcaf83effe901e543324655d8860
Autor:
George J. Bendo, Maarten Baes, Robert C. Kennicutt, Médéric Boquien, Suzanne C. Madden, Nario Kuno, Gianfranco Gentile, Christine D. Wilson, Lisa M. Young, Diane Cormier, Hiroyuki Kaneko, Jacopo Fritz, Ilse De Looze, Matthew Smith
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
De Looze, I, Baes, M, Cormier, D, Kaneko, H, Kuno, N, Young, L, Bendo, G J, Boquien, M, Fritz, J, Gentile, G, Kennicutt, R C, Madden, S C, Smith, M W L & Wilson, C D 2017, ' The interstellar medium in Andromeda's dwarf spheroidal galaxies-II. Multiphase gas content and ISM conditions ', Monthly Notices of the Royal Astronomical Society, vol. 465, no. 3, pp. 3741-3758 . https://doi.org/10.1093/mnras/stw3001
De Looze, I, Baes, M, Cormier, D, Kaneko, H, Kuno, N, Young, L, Bendo, G J, Boquien, M, Fritz, J, Gentile, G, Kennicutt, R C, Madden, S C, Smith, M W L & Wilson, C D 2017, ' The interstellar medium in Andromeda's dwarf spheroidal galaxies-II. Multiphase gas content and ISM conditions ', Monthly Notices of the Royal Astronomical Society, vol. 465, no. 3, pp. 3741-3758 . https://doi.org/10.1093/mnras/stw3001
We make an inventory of the interstellar medium material in three low-metallicity dwarf spheroidal galaxies of the Local Group (NGC147, NGC185 and NGC205). Ancillary Hi, CO, \textit{Spitzer} IRS spectra, H$\alpha$ and X-ray observations are combined
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::757760fff00c9ba0c78d6929ec1ecc83
Autor:
Vučetić, Milica M.
Publikováno v:
Универзитет у Београду
U ovoj disertaciji je analiziran uticaj zracenja ostataka supernovih (OSN) u liniji H na stopu formiranja zvezda (SFZ) odredenu na osnovu emisije u ovoj liniji. Pri- kazana je detekcija 16 optickih OSN, od strane autora ove disertacije, u delu galaks
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=nardusnacion::e58069673db21b9e1fde2380f2e6ef3c
http://nardus.mpn.gov.rs/bitstream/id/6543/Disertacija.pdf
http://nardus.mpn.gov.rs/bitstream/id/6543/Disertacija.pdf
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Journal of Astronomy and Space Sciences, Vol 25, Iss 3, Pp 245-248 (2008)
We determined values of distance modulus to nearby dwarf galaxy NGC 185 from the Tip of Red-Giant Branch (TRGB) method. Apparent magnitudes of the TRGB are estimated from the near-infrared JHK luminosity functions (LFs) of the resolved giant branch s
Autor:
Geraint F. Lewis, Annette M. N. Ferguson, J. Veljanoski, Alasdair Mackey, Nial R. Tanvir, Avon Huxor, Alan W. McConnachie, Cherie K Fishlock, Rodrigo A. Ibata, Scott Chapman, Mike Irwin
Using data from the Pan-Andromeda Archaeological Survey (PAndAS), we have discovered four new globular clusters (GCs) associated with the M31 dwarf elliptical (dE) satellites NGC 147 and NGC 185. Three of these are associated with NGC 147 and one wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69a1c7ac55d413061f868a162f133343
http://arxiv.org/abs/1308.3636
http://arxiv.org/abs/1308.3636
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.