2D Spectroscopy of IR Mergers/QSOs with galactic winds: Arp 220, Mrk 231 y NGC 4038/39

Bibcode
2003BAAA...46..108L
Lípari, S.; Mediavilla, E.; Díaz, R. J.; Taniguchi, Y.; Terlevich, R.; Dottori, H.; Zheng, W.
Bibliographical reference

Boletín de la Asociación Argentina de Astronomía, vol.46, p.108

Advertised on:
0
2003
Number of authors
7
IAC number of authors
0
Citations
0
Refereed citations
0
Description
A new part of our long term study of IR mergers and IR QSOs with galactic winds (GW) is reported. In particular, we present a study of morphology, kinematic and ionization structure of: Arp 220, Mrk 231 and NGC 4038/39. This program is based mainly on INTEGRAL two dimensional (2D) spectroscopy obtained on the 4.2 m William Herschel Telescope (at La Palma Observatory) and Fabry Perot spectroscopy obtained at 3.6 m ESO telescope. These data are combined with high resolution HST images. The properties found in IR mergers/QSOs with galactic winds mainly underline the importance of studing the possible link among: IR mergers, extreme starburst+GW, IR QSOs (with composite nature: AGN+starburst), and elliptical galaxies.
Type
Non-refereed

It may interest you

  • Non-refereed
    NIRPS near-infrared spectrograph: AITV phase at ESO3.6m/La Silla
    NIRPS is a fiber-fed AO nIR spectrograph working simultaneously with HARPS at the La Silla-ESO 3.6m telescope. The cryogenic spectrograph operating at 75K employs a cross-dispersed echelle grating (R4), covering a wavelength range of 0.98-1.80 microns in a single image using a Teledyne Hawaii-4RG infrared detector. In early 2022, the NIRPS
    Malo, Lison et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..46M
    Citations
    0
  • Non-refereed
    Transport, handling, and integration of the adaptive optics system for GTC: from the laboratory to the telescope
    The Gran Telescopio de Canarias Adaptive Optics System (GTCAO) is currently in its commissioning phase at Roque de Los Muchachos Observatory (ORM). The GTCAO is a single-conjugated post-focal system equipped with a Shack- Hartmann Wavefront Sensor (WFS) and a Deformable Mirror (DM) conjugated to the pupil, achieving a Strehl Ratio of 65% in the K
    González Carretero, Eduardo D. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..96G
    Citations
    0
  • Non-refereed
    Euclid commissioning results: the near infrared spectrometer and photometer (NISP) signal detection chain
    Euclid, the M2 mission of the ESA's Cosmic Vision 2015-2025 program, aims to explore the Dark Universe by conducting a survey of approximately 14 000 deg 2 and creating a 3D map of the observable Universe of around 1.5 billion galaxies up to redshift z ∼ 2. This mission uses two main cosmological probes: weak gravitational lensing and galaxy
    Cogato, F. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13092E..3GC
    Citations
    0