The Corona Australis Star Forming Region
| dc.creator | Neuhäuser, Ralph | |
| dc.creator | Forbrich, Jan | |
| dc.date | 2008-08-25 | |
| dc.date.accessioned | 2026-07-07T09:58:16Z | |
| dc.date.available | 2026-07-07T09:58:16Z | |
| dc.description | At a distance of about 130 pc, the Corona Australis molecular cloud complex is one of the nearest regions with ongoing and/or recent star formation. It is a region with highly variable extinction of up to AV~45 mag, containing, at its core, the Coronet protostar cluster. There are now 55 known optically detected members, starting at late B spectral types. At the opposite end of the mass spectrum, there are two confirmed brown dwarf members and seven more candidate brown dwarfs. The CrA region has been most widely surveyed at infrared wavelengths, in X-rays, and in the millimeter continuum, while follow-up observations from centimeter radio to X-rays have focused on the Coronet cluster. | |
| dc.description | 22 pages, 8 figures, to appear in the "Handbook of Star Forming Regions", ed. B. Reipurth (ASP Monograph Series) | |
| dc.identifier | https://arxiv.org/abs/0808.3374 | |
| dc.identifier | http://arxiv.org/abs/0808.3374 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/167656 | |
| dc.subject | Astrophysics | |
| dc.title | The Corona Australis Star Forming Region | |
| dc.type | text |