In:
Proceedings of the International Astronomical Union, Cambridge University Press (CUP), Vol. 15, No. S359 ( 2020-03), p. 448-449
Abstract:
We present Gemini Near-Infrared Integral-Field Spectrograph (NIFS) observations of the inner 660 × 660 pc 2 of the Seyfert 2 galaxy NGC 1125, which reveals that the emission-line profiles present two kinematic components: a narrow one (σ 〈 150 km s −1 ) due to emission of the gas in the disk and a broad component (σ 〉 150 km s −1 ) produced by a bipolar outflow, perpendicular to the galaxy’s disk.
Type of Medium:
Online Resource
ISSN:
1743-9213
,
1743-9221
DOI:
10.1017/S1743921320002379
Language:
English
Publisher:
Cambridge University Press (CUP)
Publication Date:
2020
detail.hit.zdb_id:
2170724-8
SSG:
16,12