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Necessary but not Sufficient Conditions to Trigger Starbursts CO and HI Observations of Optically-Selected Interacting Galaxies
| Content Provider | Semantic Scholar |
|---|---|
| Author | Horellou, Cathy Booth, R. S. Karlsson, Bengt |
| Copyright Year | 1999 |
| Abstract | We present the analysis of a survey of atomic and molecular gas in interacting and merging galaxies (Horellou & Booth 1997). The sample is optically selected and contains all interacting galaxies (≈ 60 systems) in a well-defined region of the Southern sky (Bergvall 1981). In order to take into account the upper limits due to non-detections, we have carried out a survival analysis. The results are compared with the ones obtained when ignoring the non-detections. We have found evidence for a lower atomic gas content per unit area in interacting galaxies compared to isolated ones. Except for a few systems with high far-infrared luminosity and correspondingly high CO fluxes, the interacting galaxies are not unusually CO-bright. The observed Hi-deficiency is therefore not due to a conversion from Hi into H2. Atomic gas from the outer part of the galaxies may have been swept by tidal interaction, or the optical extent of the galaxies may have increased due to the tidal interaction. The interacting galaxies seem to be more efficient at transforming their molecular gas into stars, as indicated by their higher LFIR/M(H2) ratio. We found no correlation between molecular gas fraction and degree of morphological distortion. |
| File Format | PDF HTM / HTML |
| Alternate Webpage(s) | http://arxiv.org/pdf/astro-ph/9910013v1.pdf |
| Language | English |
| Access Restriction | Open |
| Subject Keyword | Angular defect Booth's multiplication algorithm Distortion Galaxy Interaction Lambda calculus Sensor |
| Content Type | Text |
| Resource Type | Article |