SIMBAD references

2009MNRAS.400L..66M - Mon. Not. R. Astron. Soc., 400, L66-L70 (2009/November-3)

Lyα blobs like company: the discovery of a candidate 100kpc Lyα blob near to a radio galaxy with a giant Lyα halo B3 J2330+3927 at z = 3.1.

MATSUDA Y., NAKAMURA Y., MORIMOTO N., SMAIL I., DE BREUCK C., OHTA K., KODAMA T., INOUE A.K., HAYASHINO T., KOUSAI K., NAKAMURA E., HORIE M., YAMADA T., KITAMURA M., SAITO T., TANIGUCHI Y., TANAKA I. and HIBON P.

Abstract (from CDS):

We present the discovery of a candidate of giant radio-quiet Lyα blob (RQLAB) in a large-scale structure around a high-redshift radio galaxy (HzRG) lying in a giant Lyα halo B3J2330+3927 at redshift z = 3.087. We obtained narrow- and broad-band imaging around B3J2330+3927 with Subaru/Suprime-Cam to search for Lyα emitters (LAEs) and absorbers (LAAs) at redshift z = 3.09±0.03. We detected candidate 127 LAEs and 26 LAAs in the field of view of 31x24arcmin2 (58x44 comoving Mpc). We found that B3J2330+3927 is surrounded by a 130kpc Lyα halo and a large-scale (∼60x20 comoving Mpc) filamentary structure. The large-scale structure contains one prominent local density peak with an overdensity of greater than 5, which is 8arcmin (15 comoving Mpc) away from B3J2330+3927. In this peak, we discovered a candidate 100kpc RQLAB. The existence of both types of Lyα nebulae in the same large-scale structure suggests that giant Lyα nebulae need special large-scale environments to form. On smaller scales, however, the location of B3J2330+3927 is not a significant local density peak in this structure, in contrast to the RQLAB. There are two possible interpretations of the difference of the local environments of these two Lyα nebulae. First, RQLAB may need a prominent (δ ∼ 5) density peak of galaxies to form through intense starbursts due to frequent galaxy interactions/mergers and/or continuous gas accretion in an overdense environment. On the other hand, Lyα halo around HzRG may not always need a prominent density peak to form if the surrounding Lyα halo is mainly powered by its radio and active galactic nucleus activities. Alternatively, both RQLAB and Lyα halo around HzRG may need prominent density peaks to form but we could not completely trace the density of galaxies because we missed evolved and dusty galaxies in this survey.

Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS

Journal keyword(s): galaxies: evolution - galaxies: formation - galaxies: individual: B3J2330+3927 - cosmology: observations

VizieR on-line data: <Available at CDS (J/MNRAS/400/L66): tables1.dat tables2.dat>

Nomenclature: Table 2: [MNM2009] LAB 2330+3922. Table S1: [MNM2009] LAE NNN (Nos 1-127). Table S2: [MNM2009] LAA NN (Nos 1-26).

Simbad objects: 133

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2021.12.01-05:20:59

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