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Millimetre/Sub-millimetre Observations of Circumstellar Disks
| Content Provider | Scilit |
|---|---|
| Author | Dutrey, Anne |
| Copyright Year | 2011 |
| Description | TTauri disks located in nearby star-forming regions (e.g. Taurus-Auriga at 140 pc) are thought to be the site of planet formation, since proto-planetary disks orbiting around active (still accreting) TTauri stars should contain, in many cases, enough gas to form giant gaseous planets. As such, circumstellar disks are ideal laboratories to study planet formation, provided the gas and dust observations have enough sensitivity and resolving power. I will focus in these proceedings, on recent results of molecular observations which unveil the physical conditions of gas disks and reveal the weakness of our current understanding and modeling. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/781FDCDF35C31A333D76FFE0FF6F6B2D/S1743921311024902a.pdf/div-class-title-millimetre-sub-millimetre-observations-of-circumstellar-disks-div.pdf |
| Ending Page | 113 |
| Page Count | 11 |
| Starting Page | 103 |
| ISSN | 17439213 |
| e-ISSN | 17439221 |
| DOI | 10.1017/s1743921311024902 |
| Journal | Proceedings of the International Astronomical Union |
| Issue Number | S280 |
| Volume Number | 7 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2011-06-01 |
| Access Restriction | Open |
| Subject Keyword | Proceedings of the International Astronomical Union Astronomy and Astrophysics Protoplanetary Disks |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
