ON MASS LOSS FROM EVOLVED MASSIVE STARS
We consider stationary out flowing stellar envelopes accelerated by a radiation flux pressure. A method is developed describing a spherically symmetric flow in radiational hydrodynamics in regions with arbitrary optical depth (τ ). The solution of the derived system of differential equations is obta...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
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Odessa I. I. Mechnykov National University
2017-03-01
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| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/93017 |
| _version_ | 1818521543816249344 |
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| author | A. V. Dorodnitsyn G. S. Bisnovatyi-Kogan |
| author_facet | A. V. Dorodnitsyn G. S. Bisnovatyi-Kogan |
| author_sort | A. V. Dorodnitsyn |
| collection | DOAJ |
| description | We consider stationary out flowing stellar envelopes accelerated by a radiation flux pressure. A method is developed describing a spherically symmetric flow in radiational hydrodynamics in regions with arbitrary optical depth (τ ). The solution of the derived system of differential equations is obtained numerically. It proceeds through the singular point, where a velocity is equal to the isothermal sound speed, and satisfies zero temperature and pressure boundary conditions at the infinity. Method is discussed of self- consistent evolutionary calculations for massive stars on the stage of yellow and red supergiants, with a mass loss determined unambiguously. |
| first_indexed | 2024-12-11T01:52:28Z |
| format | Article |
| id | doaj.art-696412fe5930460dae773caf70a595ca |
| institution | Directory Open Access Journal |
| issn | 1810-4215 |
| language | English |
| last_indexed | 2024-12-11T01:52:28Z |
| publishDate | 2017-03-01 |
| publisher | Odessa I. I. Mechnykov National University |
| record_format | Article |
| series | Odessa Astronomical Publications |
| spelling | doaj.art-696412fe5930460dae773caf70a595ca2022-12-22T01:24:42ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-03-0112025025210.18524/1810-4215.1999.12.9301793017ON MASS LOSS FROM EVOLVED MASSIVE STARSA. V. Dorodnitsyn0G. S. Bisnovatyi-KoganSpace Research Institute, Profsoyuznaya st. 84/32, Moscow, RussiaWe consider stationary out flowing stellar envelopes accelerated by a radiation flux pressure. A method is developed describing a spherically symmetric flow in radiational hydrodynamics in regions with arbitrary optical depth (τ ). The solution of the derived system of differential equations is obtained numerically. It proceeds through the singular point, where a velocity is equal to the isothermal sound speed, and satisfies zero temperature and pressure boundary conditions at the infinity. Method is discussed of self- consistent evolutionary calculations for massive stars on the stage of yellow and red supergiants, with a mass loss determined unambiguously.http://oap.onu.edu.ua/article/view/93017 |
| spellingShingle | A. V. Dorodnitsyn G. S. Bisnovatyi-Kogan ON MASS LOSS FROM EVOLVED MASSIVE STARS Odessa Astronomical Publications |
| title | ON MASS LOSS FROM EVOLVED MASSIVE STARS |
| title_full | ON MASS LOSS FROM EVOLVED MASSIVE STARS |
| title_fullStr | ON MASS LOSS FROM EVOLVED MASSIVE STARS |
| title_full_unstemmed | ON MASS LOSS FROM EVOLVED MASSIVE STARS |
| title_short | ON MASS LOSS FROM EVOLVED MASSIVE STARS |
| title_sort | on mass loss from evolved massive stars |
| url | http://oap.onu.edu.ua/article/view/93017 |
| work_keys_str_mv | AT avdorodnitsyn onmasslossfromevolvedmassivestars AT gsbisnovatyikogan onmasslossfromevolvedmassivestars |