Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Dolf Michielsen"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 396:2133-2151
We present optical VLT spectroscopy of 16 dwarf elliptical galaxies (or dEs) comparable in mass to NGC 205, and belonging to the Fornax cluster and to nearby groups of galaxies. Using ULySS and STECKMAP, we derive radial profiles of the SSP-equivalen
Autor:
Frazer R. Pearce, Nigel L. Mitchell, Riccardo Brunino, Dolf Michielsen, Elizabeth J. Tasker, Stephen Hopton, Greg L. Bryan, Tom Theuns
Publikováno v:
Monthly notices of the Royal Astronomical Society
We test four commonly used astrophysical simulation codes; Enzo, Flash, Gadget and Hydra, using a suite of numerical problems with analytic initial and final states. Situations similar to the conditions of these tests, a Sod shock, a Sedov blast and
Publikováno v:
Astronomy & Astrophysics. 438:491-505
This paper is the first in a series in which we present the results of an ESO Large Program on the kinematics and internal dynamics of dwarf elliptical galaxies (dEs). We investigate the relations between the parameters that quantify the structure an
Publikováno v:
Astrophysics and Space Science. 284:635-638
Autor:
Javier Gorgas, Nicolás Cardiel, Elisa Toloba, Marc Balcells, A. Vazdekis, Alfonso Aragón-Salamanca, Christopher J. Conselice, A. J. Cenarro, Alessandro Boselli, Dolf Michielsen, Reynier Peletier, I. M. Whiley
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 385(3), 1374-1392. Oxford University Press
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Dwarf galaxies, as the most numerous type of galaxy, offer the potential to study galaxy formation and evolution in detail in the nearby Universe. Although they seem to be simple systems at first view, they remain poorly understood. In an attempt to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b524da785eb8353f106ef6661f139405
https://research.rug.nl/en/publications/da5cd6e2-432a-4ed2-974d-707814bff1b0
https://research.rug.nl/en/publications/da5cd6e2-432a-4ed2-974d-707814bff1b0
Autor:
Victor P. Debattista, Philippe Prugniel, Anna Pasquali, Ignacio Ferreras, Werner W. Zeilinger, Dolf Michielsen, Herwig Dejonghe, Mina Koleva, Sven De Rijcke
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, 2007, 670, pp.L101-L104. ⟨10.1086/524404⟩
The Astrophysical journal letters, 2007, 670, pp.L101-L104. ⟨10.1086/524404⟩
We present new estimates of ages and metallicities, based on FORS/VLT optical (4400-5500A) spectroscopy, of 16 dwarf elliptical galaxies (dE's) in the Fornax Cluster and in Southern Groups. These dE's are more metal-rich and younger than previous est
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f182fd90ff5524cc359a618e16e77d13
Publikováno v:
Proceedings of the International Astronomical Union. 2
The MAGPOP-ITP is a large observational project of the EU MAGPOP Network. In order to study the star formation history of dwarf galaxies, a total of 60 nights was allocated on the 4 large La Palma telescopes in the framework of an International Time
We present a search for CO(1->0) emission in three Local Group dwarf irregular galaxies: IC5152, the Phoenix dwarf, and UGCA438, using the ATNF Mopra radio telescope. Our scans largely cover the optical extent of the galaxies and the stripped HI clou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d398c81bab7caece7c650563637ba51
http://arxiv.org/abs/astro-ph/0609401
http://arxiv.org/abs/astro-ph/0609401
Publikováno v:
EAS Publications Series. 24:287-288
Elliptical galaxies follow a well-known luminosity – metallicity (L − Z ) relation, in the sense that more luminous ellipticals are observed to be more metal-rich than less luminous systems. Obviously this is a mass – Z relation, and its interp
Autor:
Pieter Buyle, Dolf Michielsen, Kenneth C. Freeman, Sven De Rijcke, Herwig Dejonghe, Daniel J. Pisano
Publikováno v:
Proceedings of the International Astronomical Union. 2:200-200
We present deep HI observations of a sample of 9 nearby E+A galaxies (0.05 < z < 0.1). In 7 of them, we detected up to a few times 109 M⊙ of neutral gas, making the link between E+As and early-types less direct than previously thought.