• 검색어에 아래의 연산자를 사용하시면 더 정확한 검색결과를 얻을 수 있습니다.
  • 검색연산자
검색연산자 기능 검색시 예
() 우선순위가 가장 높은 연산자 예1) (나노 (기계 | machine))
공백 두 개의 검색어(식)을 모두 포함하고 있는 문서 검색 예1) (나노 기계)
예2) 나노 장영실
| 두 개의 검색어(식) 중 하나 이상 포함하고 있는 문서 검색 예1) (줄기세포 | 면역)
예2) 줄기세포 | 장영실
! NOT 이후에 있는 검색어가 포함된 문서는 제외 예1) (황금 !백금)
예2) !image
* 검색어의 *란에 0개 이상의 임의의 문자가 포함된 문서 검색 예) semi*
"" 따옴표 내의 구문과 완전히 일치하는 문서만 검색 예) "Transform and Quantization"
쳇봇 이모티콘
ScienceON 챗봇입니다.
궁금한 것은 저에게 물어봐주세요.

논문 상세정보


Here we analyze if the ionized shells associated with giant HII regions represent the progenitors of the larger neutral hydrogen supershells detected in the Milky Way and other spiral and dwarf irregular galaxies. We calculate the evolutionary tracks that 12 HII shells found by Relano et al. (2005, 2007) would have if they expanded into the interstellar medium because of multiple supernovae explosions occurring inside the cavity. We find, contrary to Relano et al. (2007), that the evolutionary tracks of these HII shells are inconsistent with the observed parameters of the largest and most massive neutral hydrogen supershells. Thus, an additional energy source to the multiple supernovae explosions is required in order to explain the origin of the most massive neutral hydrogen shells.

참고문헌 (30)

  1. Bisnovatyi-Kogan, G. S., & SHieh, S. A. 1995, Shockwave propagation in the nonuniform interstellar medium, Rev. Mod. Phys. 67, 661 
  2. Brinks, E., 1990, The cool phase of the interstellar medium - Atomic gas, ASSL, 161, 39 
  3. Brinks, E., & Bajaja, E. 1986, A high resolution hydrogen-line survey of Messier 31. III - H I holes in the interstellar medium, A&A, 169, 14 
  4. Castor, J., McCray, R., & Weaver, R. 1975, Interstellar bubbles, ApJ, 200, 107 
  5. Chu, Y-H., & Mac Low, M.-M. 1990, X-rays from super bubbles in the Large Magellanic Cloud, ApJ, 365, 510 
  6. Ehlerova, S., & Palous, J. 2005, H I shells in the outer Milky Way, A&A, 437, 101 
  7. Hatzidimitriou, D., Stanimirovic, S., Maragoudaki, F., Stavely-Smith, L., Dapergolas, A., & Bratsolis, E. 2005, On the properties of HI shells in the Small Magellanic Cloud, MNRAS, 360, 1171 
  8. Heiles, C. 1980, Is the intercloud medium pervasive, ApJ, 235, 833 
  9. Heiles, C. 1984, H I shells, supershells, shell-like objects, and 'worms', ApJS, 55, 585 
  10. Kim, S., Dopita, M. A., Stavelet-Smith, L., & Bessel, M. 1999, HI Shells in the Large Magellanic Cloud, AJ, 118, 2797 
  11. Koo, B.-C., & McKee, C.F. 1992, Dynamics of wind bubbles and superbubbles. I - Slow winds and fast winds. II - Analytic theory, ApJ, 388, 93 
  12. Leitherer, C., Schaerer, D., Goldader, J. D., Delgado, R. M., Gonzalez, R., C., Kune, D. F., de Mello, D. F., Devost, D., & Heckman, T. M. 1999, Starburst99: Synthesis Models for Galaxies with Active Star Formation, ApJS, 123, 3 
  13. Lozinskaya, T.A. 1992, Supernova and Stellar Wind in the Interstellar Medium, (New York: American Institute of Physics), p.223 
  14. Lozinskaya, T., Moiseev, A., & Podorvanyuk, N. 2003, Detailed kinematic study of the ionized and neutral gas in the complex of star formation in the galaxy IC 1613, Astronomy Letters, 29, 77 
  15. Mashchenko, S.Y, Thilker, D.A., & Braun, R. 1999, Automated supershell recognition in spiral galaxies employing hydrodynamic simulations, A&A, 343, 352 
  16. McClure-Griffiths, N.M., Dickey, J.M., Gaensler, B.M., & Green, A. J. 2002, The galactic distribution of large H I shells, ApJ, 578, 176 
  17. McCray, R., & Kafatos, M. 1987, Supershells and propagating star formation, ApJ, 317, 190 
  18. Naze, Y., Chu, Y.-H., Points, S.D., Danforth, C.W., Rosado, M., & Chen, C.-H.R. 2001, Interstellar bubbles in two young H II regions, AJ, 122, 921 
  19. Oey, M.S., & Massey, P. 1995, Triggered star formation and the dynamics of a superbubble in the LMC: The OB association LH 47/48 in DEM 152, ApJ, 452, 210 
  20. Puche, D., Westpfahl, D., Brinks, E., & Roy, J.-R. 1992, Holmberg II - A laboratory for studying the violent interstellar medium, AJ, 103, 1841 
  21. Raga, A.C., Velazquez, P.F., Canto, J., Masciadri, E., & Rodriguez, L.F. 2001, Simulated X-ray images and spectra of the Arches cluster, ApJ, 559, 33 
  22. Relano, M., & Beckman, J.E. 2005, Expansive components in H II regions, A&A, 430, 911 
  23. Relano, M., Beckman, J.E., Daigle, O., & Carignan, C. 2007, An evolutionary sequence of expanding hydrogen shells in galaxy discs, A&A, 467, 1117 
  24. Rhode, K. L., Salzer, J. J., Westpfahl, D., & Radice, L. A. 1999, A test of the standard hypothesis for the origin of the H I holes in Holmberg II, AJ, 118, 323 
  25. Rozas, M., Beckman, J. E., & Knapen, J. H. 1996, Statistics and properties of H II regions in a sample of grand design galaxies I. Luminosity functions, A&A, 307, 735 
  26. Stevens, I.R., & Hartwell, J.M. 2003, The cluster wind from local massive star clusters, MNRAS, 339, 280 
  27. Tenorio-Tagle,G., & Bodenheimer, P. 1988, Large-scale expanding superstructures in galaxies, ARA&A, 26, 145 
  28. Valdez-Gutierrez, M., Rosado, M., Georgiev, L., Borissova, J., & Kurtev, R. 2001, Kinematics of the ionized gas in the Local Group irregular galaxy Ie 1613, A&A, 366, 35 
  29. Weaver, R., McCray, R., Castor, J., Shapiro, P., & Moore, R., 1977, Interstellar bubbles. II - Structure and evolution, ApJ, 218, 377 
  30. Mac Low, M.-M., & McCray, R. 1988, Superbubbles in disk galaxies, ApJ, 324, 776 

이 논문을 인용한 문헌 (0)

  1. 이 논문을 인용한 문헌 없음


원문 PDF 다운로드

  • ScienceON :

원문 URL 링크

원문 PDF 파일 및 링크정보가 존재하지 않을 경우 KISTI DDS 시스템에서 제공하는 원문복사서비스를 사용할 수 있습니다. (원문복사서비스 안내 바로 가기)

상세조회 0건 원문조회 0건

DOI 인용 스타일