Published July 1990
| Version v1
Report
Neutral hydrogen in the starburst galaxy NGC3690/IC694
Creators
Description
Researchers made observations of the neutral hydrogen (HI) emission structure surrounding the very deep absorption peak (observed earlier by Dickey (1986)) in the galaxy pair NGC3690/IC694. This galaxy pair is highly luminous in the far infrared, and known to exhibit extensive star formation as well as nuclear activity. Knowledge of the spatial distribution and velocity structure of the HI emission is of great importance to the understanding of the dynamics of the interaction and the resulting environmental effects on the galaxies
Additional details
Publishing Information
- Imprint Title
- The interstellar medium in external galaxies: Summaries of contributed papers
- Imprint Pagination
- 431 p.
- Journal Page Range
- p. 8-11.
- Report number
- N--91-14100
Conference
- Title
- 2. interstellar medium in external galaxies conference.
- Dates
- 3-7 Jul 1989.
- Place
- Grand Teton National Park, WY (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22061921
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- COSMIC GASES; EXPERIMENTAL DATA; FAR INFRARED RADIATION; GALAXIES; HYDROGEN; MICROWAVE SPECTRA; SPATIAL DISTRIBUTION; STAR EVOLUTION
- Descriptors DEC
- DATA; DISTRIBUTION; ELECTROMAGNETIC RADIATION; ELEMENTS; FLUIDS; GASES; INFORMATION; INFRARED RADIATION; NONMETALS; NUMERICAL DATA; RADIATIONS; SPECTRA
Optional Information
- Secondary number(s)
- NASA-CP--3084; A--90075; NAS--1.55:3084; CONF-8907237--.