Zobrazeno 1 - 10
of 186
pro vyhledávání: '"W. van Breugel"'
Autor:
Raffaella Morganti, Rene C. Vermeulen, Huub Röttgering, W. H. de Vries, R. Rengelink, W. van Breugel, Matt J. Jarvis
We present the results from our deep (16x12 hour) Westerbork Synthesis Radio Telescope (WSRT) observations of the approximately 7 square degree Bootes Deep Field, centered at 14h32m05.75s, 34d16'47.5" (J2000). Our survey consists of 42 discrete point
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd3f415441166e45b27980c670a4c22d
https://ora.ox.ac.uk/objects/uuid:59b88c62-19c1-4776-ba12-e9dd5caaa9bd
https://ora.ox.ac.uk/objects/uuid:59b88c62-19c1-4776-ba12-e9dd5caaa9bd
Publikováno v:
Astronomy & Astrophysics. 491:407-424
AGN feedback now appears as an attractive mechanism to resolve some of the outstanding problems with the "standard" cosmological models, in particular those related to massive galaxies. To directly constrain how this may influence the formation of ma
Autor:
H. J. A. Roettgering, S. A. Stanford, Andrew Zirm, Laura Pentericci, W. van Breugel, John P. Blakeslee, J. D. Kurk, Marc Postman, Piero Rosati, Bram Venemans, Ricardo Demarco, Roderik Overzier, M. Franx, G. K. Miley, A. van der Wel
Publikováno v:
The Astrophysical Journal. 680:224-231
We present new constraints on the evolution of the early-type galaxy color-magnitude relation (CMR) based on deep near-infrared imaging of a galaxy protocluster at z=2.16 obtained using NICMOS on-board the Hubble Space Telescope. This field contains
Publikováno v:
Astronomy & Astrophysics. 475:145-153
To investigate the impact of radio jets during the formation epoch of their massive host galaxies, we present an analysis of two massive, log(M_stel/ M_sun)~10.6 and 11.3, compact radio galaxies at z=3.5, TNJ0205+2242 and TNJ0121+1320. Their small ra
Autor:
Catherine A. Dukes, T. Felter, W. van Breugel, John P. Bradley, Diego F. Torres, Z. R. Dai, Giles A. Graham, Eduardo M. Bringa, Raúl A. Baragiola, Alexander G. G. M. Tielens, S. O. Kucheyev, Saša Bajt, Mark J. Loeffler
Publikováno v:
The Astrophysical Journal. 662:372-378
While a significant fraction of silicate dust in stellar winds has a crystalline structure, in the interstellar medium nearly all of it is amorphous. One possible explanation for this observation is the amorphization of crystalline silicates by relat
Publikováno v:
Astronomische Nachrichten. 327:155-158
Here we show how theoretical pan-spectral modelling is beginning to decode the physical parameters of the interstellar medium of starburst and high-redshift galaxies, is revealing the star formation rate, identifying the bolometric contribution due t
Autor:
W. H. de Vries, H. J. A. Röttgering, C. De Breuck, Michael A. Dopita, Michiel Reuland, G. K. Miley, Steve Croft, W. van Breugel
Publikováno v:
Astronomische Nachrichten. 327:175-179
We review current evidence for the existence of large emission-line halos around high redshift radio galaxies. Detailed narrow-band imaging and spectroscopic studies of these systems may help us understand the early stages of massive forming galaxies
Autor:
J. D. Kurk, C. De Breuck, Bram Venemans, H. J. A. Röttgering, Laura Pentericci, Patrick J. McCarthy, Holland C. Ford, Roderik Overzier, G. K. Miley, W. van Breugel, Timothy M. Heckman, Chris Carilli
Publikováno v:
Astronomy & Astrophysics. 431:793-812
Observations of the radio galaxy MRC 0316-257 at z=3.13 and the surrounding field are presented. Using narrow- and broad-band imaging obtained with the VLT, 77 candidate Ly-alpha emitters with a rest-frame equivalent width of > 15 A were selected in
Autor:
C. De Breuck, Laura Pentericci, W. van Breugel, Patrick J. McCarthy, H. J. A. Röttgering, Bram Venemans, Holland C. Ford, Chris Carilli, Timothy M. Heckman, G. K. Miley, Jaron Kurk
Publikováno v:
The Astrophysical Journal. 569:L11-L14
Imaging and spectroscopy with the Very Large Telescope have revealed 20 Ly? emitters within a projected distance of 1.3 Mpc and 600 km s-1 of the luminous radio galaxy TN J1338-1942 at z = 4.1. Compared to the field density of Ly? emitters, this impl
Publikováno v:
The Astrophysical Journal. 556:108-112
We present seeing-limited and adaptive optics (AO) images of the z = 1.786 radio galaxy 3C294 in the H and K' infrared bands obtained at Keck Observatory. The infrared emission of 3C294 is dominated by two distinct components separated by ~1" (9 kpc)