Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...343l..40b&link_type=abstract
Astronomy and Astrophysics, v.343, p.L40-L44 (1999)
Astronomy and Astrophysics
Astrophysics
14
Cosmology: Observations, Galaxies: Quasars: General, Galaxies: Halos, Galaxies: Clusters: General
Scientific paper
The STIS Hubble Deep Field South around the quasar J2233-606 was observed in the course of the VLT-UT1 Science Verification programme with the Test Camera in two broad-band filters, B and R, and in a narrow-band filter roughly centered at the quasar emission redshift, z_em = 2.238. The most striking result is the discovery of a giant Lyalpha nebulosity around this radio-weak quasar, with an overall extent of 9.2('') x 12.1('') or 121 x 159 h50(-2) kpc(2) and a luminosity of 3.1 x 10(44) h50(-2) erg s(-1) (for q_0 = 0), similar to those found around radio-loud quasars and radio galaxies. There are three additional emission-line candidates in a 1.11(') x 1.24(') field with an observed Lyalpha flux above our 3sigma Lyalpha detection limit of 1.9 x 10(-17) erg s(-1) cm(-2) for point sources. The resolved bright object located 4.9('') north-east of the quasar, which has recently been identified as a galaxy at z_g = 0.57, has an associated, weak Mg ii absorption in the quasar spectrum. Based on observations collected at the European Southern Observatory, Paranal, Chile.
Arnouts Stephane
Bergeron Jacqueline
Bresolin Fabio
Cristiani Stefano
Fasano Giancarmine
No associations
LandOfFree
Lyalpha emission at Z ~ z_em around the quasar J2233-606 in the Hubble Deep Field South does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Lyalpha emission at Z ~ z_em around the quasar J2233-606 in the Hubble Deep Field South, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Lyalpha emission at Z ~ z_em around the quasar J2233-606 in the Hubble Deep Field South will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1442465