THE NATURE OF STARS WITH THE B[E] PHENOMENON THROUGH INTERFEROMETRIC EYES
The recently dened Galactic FSCMa group comprises -40 not very luminous objects that signicantly expand the luminosity range of hot dust-forming stars. These objects exhibit extremely strong emission-line spectra and IR excesses, which are indicative of compact dust envelopes. They are most likely b...
שמור ב:
| הוצא לאור ב: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| מחבר ראשי: | |
| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
Universidad Nacional Autónoma de México
2010
|
| נושאים: | |
| גישה מקוונת: | https://www.redalyc.org/articulo.oa?id=57115706036 |
| תגים: |
אין תגיות, היה/י הראשונ/ה לתייג את הרשומה!
|