Zobrazeno 1 - 2
of 2
pro vyhledávání: '"H. J. Mc Cracken"'
Autor:
M. Creze, O. Le Fevre, Céline Reylé, Yannick Mellier, Jean-Charles Cuillandre, H. J. Mc Cracken, Annie C. Robin, V. Mohan
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2004, 426, pp.65-73. ⟨10.1051/0004-6361:20040491⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 426, pp.65-73
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 426, pp.65-73. ⟨10.1051/0004-6361:20040491⟩
Astronomy and Astrophysics-A&A, 2004, 426, pp.65-73. ⟨10.1051/0004-6361:20040491⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 426, pp.65-73
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 426, pp.65-73. ⟨10.1051/0004-6361:20040491⟩
Having ruled out the possibility that stellar objects are the main contributor of the dark matter embedding galaxies, microlensing experiments cannot exclude the hypothesis that a significant fraction of the Milky Way dark halo might be made of MACHO
Autor:
M. Pannella, C. L. Carilli, E. Daddi, H. J. Mc Cracken, F. Owen, A. Renzini, E. Schinnerer, V. Smolčić, Giuliana Giobbi, Amedeo Tornambe, Gabriella Raimondo, Marco Limongi, L. A. Antonelli, Nicola Menci, Enzo Brocato
We present preliminary results of a study aimed to constrain the star formation rate and dust content of galaxies as a function of mass at z≈ 2,, a crucial time for galaxy evolution: this is the cosmic epoch when most of the stars in the Universe a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab5aee53eb11780c6c570b1aa7212498
https://resolver.caltech.edu/CaltechAUTHORS:20160505-154751576
https://resolver.caltech.edu/CaltechAUTHORS:20160505-154751576