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http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2663Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.creator | Moro-Martín, A. | - |
| dc.creator | Noriega-Crespo, A. | - |
| dc.creator | Molinari, S. | - |
| dc.creator | Testi, Leonardo | - |
| dc.creator | Cernicharo, José | - |
| dc.creator | Sargent, A. | - |
| dc.date | 2008-01-09T16:06:18Z | - |
| dc.date | 2008-01-09T16:06:18Z | - |
| dc.date | 2001-03-05 | - |
| dc.date.accessioned | 2017-01-31T00:59:39Z | - |
| dc.date.available | 2017-01-31T00:59:39Z | - |
| dc.identifier | arXiv:astro-ph/0103065v1 | - |
| dc.identifier | http://hdl.handle.net/10261/2663 | - |
| dc.identifier.uri | http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2663 | - |
| dc.description | The Cepheus E outflow has been studied in the mid and far infrared using the ISO CAM and LWS instruments, and at millimetric wavelengths using OVRO. In the near and mid-IR, its morphology is similar to that expected for a jet driven outflow, where the leading bow shocks entrain and accelerate the surrounding molecular gas. As expected, fine structure atomic/ionic emission lines arise from the bow shocks, at both the Mach Disk and the stagnation tip, where J-shocks are dominant. The H2, H2O and CO molecular emission could arise further `downstream' at the bow shock wings where the shocks (v = 8-35 km/s) are oblique and more likely to be C-type. The 13CO emission arises from entrained molecular gas and a compact high velocity emission is observed, together with an extended low velocity component that almost coincides spatially with the H2 near-IR emission. The millimetric continuum emission shows two sources. We identify one of them with IRAS 23011+6126, postulating is the driver of the Cepheus E outflow; the other, also an embedded source, is likely to be driving one of other outflows observed in the region. | - |
| dc.description | Peer reviewed | - |
| dc.format | 710901 bytes | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.relation | Preprint | - |
| dc.rights | openAccess | - |
| dc.subject | Stars: formation | - |
| dc.subject | Stars: pre-main-sequence | - |
| dc.subject | ISM: jets and outflows | - |
| dc.subject | Infrared: ISM: lines and bands | - |
| dc.title | Infrared and Millimetric Study of the Young Outflow Cepheus E | - |
| dc.type | Pre-print | - |
| Appears in Collections: | Digital Csic | |
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