쌍방분자분출역과 항성제트 간의 역학적 구조 및 항성생성에 관한 연구
(주)코리아스칼라
- 최초 등록일
- 2023.04.05
- 최종 저작일
- 1989.06
- 21페이지/ 어도비 PDF
- 가격 5,700원
* 본 문서는 배포용으로 복사 및 편집이 불가합니다.
서지정보
ㆍ발행기관 : 한국지구과학회
ㆍ수록지정보 : 한국지구과학회지 / 10권 / 1호
ㆍ저자명 : 최승언, 정현철
영어 초록
The proposed evaporation disk model is improved to figure out two flow system ~n the observed bipolar molecular outflow and stellar optical jet. Using the improved model, we can interpret the dymanical interactions of the two flows as well as obtain the physical parameter distributions along the flows Numerical & analytical adiabatic hydrodynamic calculations of the stellar jet inside show that the jet Mach number increases with an inversely proportional to the jet radius and M₁∼35, V₁∼150㎞/sec, Z₁∼0.1 pc, R₁∼0.05pc, T₁∼10³K, ρ₁-4.3×10^(-3)g/㎤(n₁∼25/㎤) at the end of the flow. By the way, in the case of the molecular flow. which is developed from the evaporated disk wind, the same calculations show that the flow Mach number increases with an inversely proportional to the mass flux distribution and M_d∼15, V₁∼15㎞/sec, Z_d∼1pc, R_d∼025pc, T_d∼10²K, ρ_d∼4.0×10^(-3)g/㎤(n_d∼25/㎤) at the flow end Most of the calculated physical parameters in the two flows consistent with the observational ones very well. The theoretically calculated flows develope the supersonic flows to make the shocked regions at the ends of flows. These regions are gravitationally unstable to produced the fragmentations whose masses are∼2 M- in the stellar let case and 0.3 M_⊙ in the bipolar flow case. This mass distribution supports that both the origins of Herbig-Haro objects and the birth of low mass stars are attributed to the instabilities of the shocked regions in the stellar jets and the bipolar molecular flows respectively.
참고 자료
없음
"한국지구과학회지"의 다른 논문
더보기 (4/9)