Studying the Dynamics of Star Forming and IR Luminous Galaxies with Infrared Spectroscopy
With the advent of efficient near-IR spectrometers on 10m-class telescopes, exploiting the new generation of low readout noise, large format detectors, OH avoidance and sub-arcsecond seeing, 1-2.4 micron spectroscopy is becoming a key means of obtaining detailed galaxy dynamics and for studies of hi...
| Main Authors: | , , , , , , |
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| Format: | Conference item |
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2002
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| _version_ | 1797057563700756480 |
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| author | Genzel, R Tacconi, L Barden, M Lehnert, MD Lutz, D Rigopoulou, D Thatte, N |
| author_facet | Genzel, R Tacconi, L Barden, M Lehnert, MD Lutz, D Rigopoulou, D Thatte, N |
| author_sort | Genzel, R |
| collection | OXFORD |
| description | With the advent of efficient near-IR spectrometers on 10m-class telescopes, exploiting the new generation of low readout noise, large format detectors, OH avoidance and sub-arcsecond seeing, 1-2.4 micron spectroscopy is becoming a key means of obtaining detailed galaxy dynamics and for studies of high-z galaxies. In the following we present the results of three recent IR spectroscopy studies on the dynamics of ULIRG mergers, super star clusters in the Antennae, and on the properties of the rotation curves of z~1 disk galaxies, carried out with ISAAC on the VLT and NIRSPEC on the Keck. |
| first_indexed | 2024-03-06T19:38:14Z |
| format | Conference item |
| id | oxford-uuid:1fc2447c-6df8-4a5d-a1e9-bd4b2176e48e |
| institution | University of Oxford |
| last_indexed | 2024-03-06T19:38:14Z |
| publishDate | 2002 |
| record_format | dspace |
| spelling | oxford-uuid:1fc2447c-6df8-4a5d-a1e9-bd4b2176e48e2022-03-26T11:23:46ZStudying the Dynamics of Star Forming and IR Luminous Galaxies with Infrared SpectroscopyConference itemhttp://purl.org/coar/resource_type/c_5794uuid:1fc2447c-6df8-4a5d-a1e9-bd4b2176e48eSymplectic Elements at Oxford2002Genzel, RTacconi, LBarden, MLehnert, MDLutz, DRigopoulou, DThatte, NWith the advent of efficient near-IR spectrometers on 10m-class telescopes, exploiting the new generation of low readout noise, large format detectors, OH avoidance and sub-arcsecond seeing, 1-2.4 micron spectroscopy is becoming a key means of obtaining detailed galaxy dynamics and for studies of high-z galaxies. In the following we present the results of three recent IR spectroscopy studies on the dynamics of ULIRG mergers, super star clusters in the Antennae, and on the properties of the rotation curves of z~1 disk galaxies, carried out with ISAAC on the VLT and NIRSPEC on the Keck. |
| spellingShingle | Genzel, R Tacconi, L Barden, M Lehnert, MD Lutz, D Rigopoulou, D Thatte, N Studying the Dynamics of Star Forming and IR Luminous Galaxies with Infrared Spectroscopy |
| title | Studying the Dynamics of Star Forming and IR Luminous Galaxies with
Infrared Spectroscopy |
| title_full | Studying the Dynamics of Star Forming and IR Luminous Galaxies with
Infrared Spectroscopy |
| title_fullStr | Studying the Dynamics of Star Forming and IR Luminous Galaxies with
Infrared Spectroscopy |
| title_full_unstemmed | Studying the Dynamics of Star Forming and IR Luminous Galaxies with
Infrared Spectroscopy |
| title_short | Studying the Dynamics of Star Forming and IR Luminous Galaxies with
Infrared Spectroscopy |
| title_sort | studying the dynamics of star forming and ir luminous galaxies with infrared spectroscopy |
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