Sub-Arcsecond CO(1–0) and CO(2–1) Observations of the Ultraluminous Infrared Galaxy IRAS 10190+1322

Astronomy and Astrophysics - France
doi 10.1051/0004-6361:20077448
Full Text
Abstract

Available in full text

Date
Authors
Publisher

EDP Sciences

Related search

Resolved CO (1 → 0) Nuclei in IRAS 14348−1447: Evidence for Massive Bulge Progenitors to Ultraluminous Infrared Galaxies

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2000English

5.12. High-Resolution CO (1-0) Observations of the Ringed Galaxy NGC 4736

Symposium - International Astronomical Union
1998English

CO (2–1) Observations of Maffei 2

Symposium - International Astronomical Union
1985English

ALMA CO(2-1) Observations in the XUV Disk of M83

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Discovery of an X-Ray Quasar Wind Driving the Cold Gas Outflow in the Ultraluminous Infrared Galaxy IRAS F05189-2524

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

New Observations and a New Interpretation of CO(3–2) in IRAS F10214+4724

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
1995English

An Ultraluminous IRAS Galaxy With an Extremely Soft X-Ray Spectrum

International Astronomical Union Colloquium
1997English

Alkali/TX[sub 2] Catalysts for CO/H[sub 2] Conversion to C[sub 1]-C[sub 4] Alcohols

1989English

CO Observations of the Interacting Galaxy Pair NGC 5394/95

Astronomical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2002English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy