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한국천문학회지

1968년 ~ 2025년까지 1,227 건한국천문학회지를 격월간 확인하실 수 있습니다.

  • The Korean Astronomical Society (The Korean Astronomical Society)
  • 계간 (Quarterly)
  • ISSN : 1225-4614 (ISSN : 1225-4614)
  • DB구축현황 : 1,227건 (DB Construction : 1,227 Articles)
안내사항
총 게시글 1,227 페이지 100/123
991
  • KIM JONGSOO
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.167-168
  • 1996
  • 원문 바로보기
992
  • YIM Jo RYEONG
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.241-242
  • 1996
  • 원문 바로보기
The UBV observations of the close binary system CW Cephei were made from August 198:3 to December 1984 during 25 nights using the 61cm Boller and Chivens reflector at the Sobaeksan Astronomy Observatory. The new UBV light curves were analyzed with the recent Wilson-Devinney binary model. Our photometric solution for CW Cep were well consistent with those of Clausen &. Gimenez (1991). Using our photometric solution and Popper & Hill (1991) spectroscopic one, each absolute masses and radii of components for CW Cep were derived as 13.63 M<TEX>$\bigodot$</TEX> and 5.83 R<TEX>$\bigodot$</TEX> for the primary, and 12.18 M<TEX>$\bigodot$</TEX> and 5.14 R<TEX>$\bigodot$</TEX> for the secondary, respectively.
993
  • ISOBE SYUZO
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.451-453
  • 1996
  • 원문 바로보기
There is a question, 'Which is beautiful, a flower or a star?'. Its answer is different from one person .to another. It is only a matter of what one is interested in. It is very difficult for most school pupils, who will have non-scientific jobs, to understand science courses taught currently in school, because each science (physics, chemistry, biology, and earth science) is independently taught from the other sciences. Therefore, their knowledge of sciences obtained during their school period does not significantly help their understanding of global environmental problems. I am proposing that several scientific stories should be prepared to connect all the related scientific phenomena in order to give those pupils ideas in understanding global environmental problems. I believe that astronomy is able to play an important role in this context.
994
  • NHA SARAH
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.243-243
  • 1996
  • 원문 바로보기
UBV observations have been made jointly at three observatories for the recent eclipse of the long period atmospheric eclipsing binary star Zeta Aur in 1995-6. Observations covered successfully the phases before, during, and after the eclipse enable us to determine the accurate time of mid-eclipse and the duration of the totality. The hypothesis of the expansion of the K supergiant has been tested and the positive conclusion may be derived.
995
  • CHAKRABARTI SANDIP K.
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.229-230
  • 1996
  • 원문 바로보기
996
  • ANDERSEN J.
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.239-240
  • 1996
  • 원문 바로보기
Precise masses, radii, and luminosities from eclipsing binaries and colour-magnitude diagrams for open clusters are classic tools in empirical tests of stellar evolution models. We review the accuracy and completeness required for such data to discriminate between current models and describe some recent. results with implications for convection theory.
997
  • NARLIKAR JAYANT V.
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.1-5
  • 1996
  • 원문 바로보기
Recent discussions of observational constraints on the standard hot big bang model are reviewed and it is argued that now there is room for considering alternative cosmologies. The quasi-steady state cosmology is briefly described. This model seems to explain most of the observed features of the universe, including the m-z relation, radio source count, the light nuclear abundances and the microwave background.
998
  • EHGAMBERDIEV SH. A.
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.287-289
  • 1996
  • 원문 바로보기
IRIS(International Research on the Interior of the sun) is the name of a worldwide network of 6 stations for whole disc Doppler shift measurements. The network has been operating since 1987 and by now a few series of a hundred days long unbroken (by day/night periodicity) data were received. Analysis of these data allowed to receivesome new results which are discussed in the paper.
999
  • RYU DONGSU
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.25-26
  • 1996
  • 원문 바로보기
In the standard theory of the large scale structure formation, matter accretes onto high density perturbations via gravitational instability. Collision less dark matter forms caustics around such structures, while collisional baryonic matter forms accretion shocks which then halt and heat the infalling gas. Here we discuss the characteristics. roles, and observational consequences of these accretion shocks.
1000
  • LYO A-RAN
  • Journal of the Korean astronomical society = 천문학회지
  • 29, n.suppl1
  • pp.65-66
  • 1996
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