Results 161 to 170 of about 218 (186)
Lyman α emitters, Lyman break galaxies and elliptical galaxies
Lyman α emitters, Lyman break galaxies and elliptical galaxiesopenaire +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Annual Review of Astronomy and Astrophysics, 2002
▪ Abstract In this paper we review the properties of Lyman-break galaxies, namely starburst galaxies at high redshifts, approximately in the range 2.5 < z < 5, identified by the colors of their far ultraviolet spectral energy distribution around the 912 Å Lyman continuum discontinuity.
Mauro Giavalisco
exaly +2 more sources
▪ Abstract In this paper we review the properties of Lyman-break galaxies, namely starburst galaxies at high redshifts, approximately in the range 2.5 < z < 5, identified by the colors of their far ultraviolet spectral energy distribution around the 912 Å Lyman continuum discontinuity.
Mauro Giavalisco
exaly +2 more sources
Faint Lyman-break galaxies as a crucial test for galaxy formation models [PDF]
Monthly Notices of the Royal Astronomical Society, 2009 17 pages, 13 figures, 1 table; accepted for publication by ...
Eros Vanzella +2 more
exaly +5 more sources
Are High-Redshift Damped Lyα Galaxies Lyman Break Galaxies?*
Astrophysical Journal, 2002 We use deep HST STIS and NICMOS images of three spectroscopically confirmed galaxy counterparts of high-redshift damped Ly? (DLA) absorbers (one of which is a new discovery) to test the hypothesis that high-redshift DLA galaxies are Lyman break galaxies. If this hypothesis is correct, the emission properties of DLA galaxies must lie within the range of
Peter Jakobsen, Palle Moller
exaly +2 more sources
High Redshift Lyman Break Galaxies
2006Two of the most outstanding issues in modern astrophysics are what reionized the Universe and how did the first objects form. Observations of galaxies selected through the Lyman-Break technique indicate that UV photon output at the end of reionization was dominated by relatively faint low mass galaxies and not AGN.
Lehnert, M., Bremer, M.
openaire +2 more sources
Lyman break galaxies as collisional starbursts
Second international workshop on particle physics and the early universe (COSMO-98), 1999The nature of the galaxies recently discovered at redshift [1,2] z≳3, when the Universe was only about two billion years old, is an intriguing puzzle. They are forming stars at a high rate, comparable to local “starburst” galaxies [3], but while the latter are relatively rare, the high-z galaxies are as numerous as local normal galaxies.
J. Bullock +9 more
openaire +1 more source
The 9th astrophysics conference: After the dark ages, when galaxies were young (the Universe at 2<Z<5), 1999
James D. Lowenthal, L. Simard, D. Koo
openaire +1 more source
James D. Lowenthal, L. Simard, D. Koo
openaire +1 more source
Massive black holes in high-redshift Lyman Break Galaxies
Monthly Notices of the Royal Astronomical Society, 2021Simona Gallerani, Andrea Ferrara
exaly
Lyman Break Galaxies: A Ten-year Perspective
Il Nuovo Cimento B, 2007Pettini, M +8 more
openaire +2 more sources
Detailed astrophysical properties of Lyman Break Galaxies
2003A large statistical sample of z~3 galaxies has been efficiently UV-color-selected, and confirmed spectroscopically. Here we present additional observations providing insight into the physical conditions in these Lyman Break Galaxies (LBGs), selected to be rapidly forming stars when the universe was ~15% of its current age.
openaire +1 more source