Photoabsorption of X-Rays in the Magnetic Compact Star

Radiation due to accretion from an accretion disc around the intermediate polars and photoabsorption of this radiation in the accretion funnel have been taken into account as a phenomenological model to study the physics of the magnetic funnel in the magnetic compact star. The first results show tha...

Full description

Bibliographic Details
Main Author: Yonggi Kim
Format: Article
Language:English
Published: The Korean Space Science Society 1992-12-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n2/OJOOBS_1992_v9n2_171.pdf
_version_ 1797368930697740288
author Yonggi Kim
author_facet Yonggi Kim
author_sort Yonggi Kim
collection DOAJ
description Radiation due to accretion from an accretion disc around the intermediate polars and photoabsorption of this radiation in the accretion funnel have been taken into account as a phenomenological model to study the physics of the magnetic funnel in the magnetic compact star. The first results show that such a model scenario can be used to estimate some parameters in these systems. Some constraints of this model regarding to the observational data of one intermediate polar, EX Hya, are also discussed.
first_indexed 2024-03-08T17:39:42Z
format Article
id doaj.art-390ae9e386c649268af83c747c446a5c
institution Directory Open Access Journal
issn 2093-5587
2093-1409
language English
last_indexed 2024-03-08T17:39:42Z
publishDate 1992-12-01
publisher The Korean Space Science Society
record_format Article
series Journal of Astronomy and Space Sciences
spelling doaj.art-390ae9e386c649268af83c747c446a5c2024-01-02T11:13:04ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14091992-12-0192171182Photoabsorption of X-Rays in the Magnetic Compact StarYonggi Kim0Yonsei University Observatory, Seoul 120-749, KoreaRadiation due to accretion from an accretion disc around the intermediate polars and photoabsorption of this radiation in the accretion funnel have been taken into account as a phenomenological model to study the physics of the magnetic funnel in the magnetic compact star. The first results show that such a model scenario can be used to estimate some parameters in these systems. Some constraints of this model regarding to the observational data of one intermediate polar, EX Hya, are also discussed.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n2/OJOOBS_1992_v9n2_171.pdf
spellingShingle Yonggi Kim
Photoabsorption of X-Rays in the Magnetic Compact Star
Journal of Astronomy and Space Sciences
title Photoabsorption of X-Rays in the Magnetic Compact Star
title_full Photoabsorption of X-Rays in the Magnetic Compact Star
title_fullStr Photoabsorption of X-Rays in the Magnetic Compact Star
title_full_unstemmed Photoabsorption of X-Rays in the Magnetic Compact Star
title_short Photoabsorption of X-Rays in the Magnetic Compact Star
title_sort photoabsorption of x rays in the magnetic compact star
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n2/OJOOBS_1992_v9n2_171.pdf
work_keys_str_mv AT yonggikim photoabsorptionofxraysinthemagneticcompactstar