E-viri
Recenzirano
-
Cox, P; Krips, M; Neri, R; Omont, A; Güsten, R; Menten, K. M; Wyrowski, F; Weiß, A; Beelen, A; Gurwell, M. A; Dannerbauer, H; Ivison, R. J; Negrello, M; Aretxaga, I; Hughes, D. H; Auld, R; Baes, M; Blundell, R; Buttiglione, S; Cava, A; Cooray, A; Dariush, A; Dunne, L; Dye, S; Eales, S. A; Frayer, D; Fritz, J; Gavazzi, R; Hopwood, R; Ibar, E; Jarvis, M; Maddox, S; Michałowski, M; Pascale, E; Pohlen, M; Rigby, E; Smith, D. J. B; Swinbank, A. M; Temi, P; Valtchanov, I; van der Werf, P; de Zotti, G
The Astrophysical journal, 10/2011, Letnik: 740, Številka: 2Journal Article
We report ground-based follow-up observations of the exceptional source, ID 141, one of the brightest sources detected so far in the Herschel Astrophysical Terahertz Large Area Survey cosmological survey. ID 141 was observed using the IRAM 30 m telescope and Plateau de Bure interferometer (PdBI), the Submillimeter Array, and the Atacama Pathfinder Experiment submillimeter telescope to measure the dust continuum and emission lines of the main isotope of carbon monoxide and carbon (C I and C II). The detection of strong CO emission lines with the PdBI confirms that ID 141 is at high redshift (z = 4.243 ? 0.001). The strength of the continuum and emission lines suggests that ID 141 is gravitationally lensed. The width ( Delta *DV FWHM ~ 800 km s--1) and asymmetric profiles of the CO and carbon lines indicate orbital motion in a disk or a merger. The properties derived for ID 141 are compatible with an ultraluminous (L FIR ~ (8.5 ? 0.3) X 1013 Delta *m--1 L L , where Delta *mL is the amplification factor), dense (n 104 cm--3), and warm (T kin 40 K) starburst galaxy, with an estimated star formation rate of (0.7-1.7) X 104 Delta *m--1 L M yr--1. The carbon emission lines indicate a dense (n 104 cm--3) photon-dominated region, illuminated by a far-UV radiation field a few thousand times more intense than that in our Galaxy. In conclusion, the physical properties of the high-z galaxy ID 141 are remarkably similar to those of local ultraluminous infrared galaxies.
Avtor
Vnos na polico
Trajna povezava
- URL:
Faktor vpliva
Dostop do baze podatkov JCR je dovoljen samo uporabnikom iz Slovenije. Vaš trenutni IP-naslov ni na seznamu dovoljenih za dostop, zato je potrebna avtentikacija z ustreznim računom AAI.
Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
---|---|---|---|---|---|---|---|---|
JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
Baze podatkov, v katerih je revija indeksirana
Ime baze podatkov | Področje | Leto |
---|
Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
---|
Vir: Osebne bibliografije
in: SICRIS
To gradivo vam je dostopno v celotnem besedilu. Če kljub temu želite naročiti gradivo, kliknite gumb Nadaljuj.