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Far-infrared Excesses in Classical Be Stars
| Content Provider | Scilit |
|---|---|
| Author | Miroshnichenko, A. S. Bjorkman, K. S. |
| Copyright Year | 2000 |
| Description | A sample of Be stars with large far-infrared excesses detected by IRAS is selected and their high-resolution IRAS images are examined. The far-infrared emission from most of them is marginally extended and is associated with the optical sources. Modeling of the stars’ spectral energy distributions allows us to rule out the infrared cirrus nature of the excesses. We suggest that the excesses are more likely due to circumstellar dust, possibly formed early in the evolution of the star. |
| Related Links | https://www.cambridge.org/core/services/aop-cambridge-core/content/view/FED3110144CBBE8F09525198CF18F37B/S0252921100056311a.pdf/div-class-title-far-infrared-excesses-in-classical-be-stars-div.pdf |
| Ending Page | 487 |
| Page Count | 4 |
| Starting Page | 484 |
| ISSN | 02529211 |
| DOI | 10.1017/s0252921100056311 |
| Journal | International Astronomical Union Colloquium |
| Volume Number | 175 |
| Language | English |
| Publisher | Cambridge University Press (CUP) |
| Publisher Date | 2000-01-01 |
| Access Restriction | Open |
| Subject Keyword | International Astronomical Union Colloquium Astronomy and Astrophysics Infrared Excesses |
| Content Type | Text |
| Resource Type | Article |