- PII
- S30345170S0004629925020015-1
- DOI
- 10.7868/S3034517025020015
- Publication type
- Article
- Status
- Published
- Authors
- Volume/ Edition
- Volume 102 / Issue number 2
- Pages
- 85-95
- Abstract
- UBVRcIc observations of microquasar SS 433 from 1980 to 2023 revealed a stable effect unusual for classical eclipsing binary systems. In the phases of maximum accretion disk opening, the depths of the primary and secondary eclipsing minima of the orbital light curve decrease synchronously with increasing wavelength. To explain this effect, we have used the model of an eclipsing binary system in which there is a third non- eclipsing light. We show that the main source of the third light at a mass-loss rate of 10−4
- Keywords
- индивидуальные звезды тесные двойные затменные звезды аккреционные диски
- Date of publication
- 01.02.2025
- Year of publication
- 2025
- Number of purchasers
- 0
- Views
- 72
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