GEMINI 3D spectroscopy of BAL+IR+Fe II QSOs: II. IRAS 04505-2958 an explosive QSO with hypershell and a new scenario for galaxy formation and galaxy end
Lipari, S.; Bergmann, M.; Sanchez, S. F.;Garcia-Lorenzo, B.; Terlevich, R.; Mediavilla, E.;Taniguchi, Y.; Zheng, W.; Punsly, B.; Jahnke, K.;Ahumada, A.; Merlo, D.. GEMINI 3D spectroscopy of BAL+IR+Fe II QSOs: II. IRAS 04505-2958 an explosive QSO with hypershell and a new scenario for galaxy formation and galaxy end. eprint arXiv:0901.3292. 2009, Vol. , p. -2009.
From a study of BAL + IR + Fe II QSOs (using deep Gemini GMOS-IFU
spectroscopy) new results are presented: for IRAS 04505-2958.
Specifically, we have studied in detail the out flow (OF) process and
their associated structures, mainly at two large galactic scales: (i)
two blobs/shells (S1, S2) at radius r = 1.1 and 2.2 kpc; and (ii) an
external hypergiant shell (S3) at r = 11 kpc. In addition, the presence
of two very extended hypergiant shells (S4, S5) at r = 80 kpc is
discussed. From this GMOS study the following main results were
obtained: (i) For the external hypergiant shell S3 the kinematics GMOS
maps of the ionized gas show very similar features to those observed for
the prototype of exploding external supergiant shell: in NGC 5514. (ii)
The main knots K1, K2 and K3 -of this hypergiant shell S3- show a
stellar population and emission line ratios associated with the presence
of a starburst + OF/shocks. (iii) The internal shells S1 and S2 show
structures, OF components and properties very similar to those detected
in the nuclear shells of Mrk 231. (iv) The shells S1+S2 and S3 are
aligned at PA = 131: i.e. suggesting that the OF process is in the
blow-out phase with bipolar structure. In addition, the shells S4 and S5
(at 80-100 kpc scale) are aligned at PA = 40, i.e.: a bipolar OF
perpendicular to the internal OF. Finally, the generation of UHE cosmic
rays and neutrino/ dark-matter -associated with HyNe in BAL + IR + Fe II
QSOs- is discussed.
From a study of BAL + IR + Fe II QSOs (using deep Gemini GMOS-IFU
spectroscopy) new results are presented: for IRAS 04505-2958.
Specifically, we have studied in detail the out flow (OF) process and
their associated structures, mainly at two large galactic scales: (i)
two blobs/shells (S1, S2) at radius r = 1.1 and 2.2 kpc; and (ii) an
external hypergiant shell (S3) at r = 11 kpc. In addition, the presence
of two very extended hypergiant shells (S4, S5) at r = 80 kpc is
discussed. From this GMOS study the following main results were
obtained: (i) For the external hypergiant shell S3 the kinematics GMOS
maps of the ionized gas show very similar features to those observed for
the prototype of exploding external supergiant shell: in NGC 5514. (ii)
The main knots K1, K2 and K3 -of this hypergiant shell S3- show a
stellar population and emission line ratios associated with the presence
of a starburst + OF/shocks. (iii) The internal shells S1 and S2 show
structures, OF components and properties very similar to those detected
in the nuclear shells of Mrk 231. (iv) The shells S1+S2 and S3 are
aligned at PA = 131: i.e. suggesting that the OF process is in the
blow-out phase with bipolar structure. In addition, the shells S4 and S5
(at 80-100 kpc scale) are aligned at PA = 40, i.e.: a bipolar OF
perpendicular to the internal OF. Finally, the generation of UHE cosmic
rays and neutrino/ dark-matter -associated with HyNe in BAL + IR + Fe II
QSOs- is discussed.