簡易檢索 / 詳目顯示

研究生: 江奕寬
Chiang, Yi-Kuan
論文名稱: THE LONG-TERM VARIABILITY OF THE X-RAY SOURCES IN M82
星系M82中X光源的長時間尺度變化
指導教授: 江國興
Kong, Albert K.H.
口試委員:
學位類別: 碩士
Master
系所名稱: 理學院 - 天文研究所
Institute of Astronomy
論文出版年: 2009
畢業學年度: 97
語文別: 英文
論文頁數: 63
中文關鍵詞: 天文X光星系
外文關鍵詞: Astronomy, X-ray, Galaxy
相關次數: 點閱:2下載:0
分享至:
查詢本校圖書館目錄 查詢臺灣博碩士論文知識加值系統 勘誤回報
  • 本論文研究星系M82中X光源在長時間尺度下的變化。透過分析自1999至2007年間9個錢卓拉X光望遠鏡對M82觀測的資料,我們在M82內偵測到58個亮度約大於1037 ergs s-1 的X光點光源。在這58個X光源中,我們發現了三個可能與超星星殘骸有關的X光源,以及一個超軟X光源。在長時間尺度下,29個X光源有亮度的變化,3個X光源有光譜的變化。更進一步的,我們將29個X光源歸類為變星,8個歸類為恆定光源。在這29個變星之中,有20個光源的光度變化比率大於3倍,有6個變化劇烈的光源被歸類為瞬變現象。星系M82中,54%的X光源在長時間尺度下的光度變化比率大於3倍,與其他星系相較之下,這樣的光變是極為強烈的。如此強烈的長時間尺度光變,意味著在M82中的X光源大多為X光雙星。此外,我們發現M82中的一個超新星SN 2004am,在超新星爆炸後的幾年內,X光亮度穩定增加。截至目前為止,只有兩個超新星,SN 1996cr和SN 1987A被觀測到類似的現象。透過研究與比較這三個超新星,也許可以推知環繞超新星物質的密度以及其結構。探知SN 2004am的本質可以增加我們對II型超新星末期演化的了解。因此,我們對錢卓拉X光望遠鏡提出一個觀測提案,藉以更進一步的研究超新星SN 2004am。


    We investigate the long-term variability exhibited by the X-ray point sources in the starburst galaxy M82. By combining 9 Chandra observations taken between 1999 and 2007, we detect 58 X-ray point sources within the D25 isophote of M82 down to a luminosity of ~ 1037 ergs s-1. Of these 58 sources, we identify 3 supernova remnant candidates and one supersoft source. Twenty-nine sources in M82 exhibit long-term (i.e., days to years) flux variability and 3 show long-term spectral variability. Furthermore, we classify 29 sources as variables and 8 as persistent sources. Among the total 29 variables, 20 varied by a flux ratio of > 3 and 6 are transient candidates. By comparing with other nearby galaxies, M82 shows extremely strong long-term X-ray variability that 54% of the X-ray sources are variables with a flux ratio of > 3. The strong X-ray variability of M82 suggests that the population is dominated by X-ray binaries. Besides, one of the X-ray supernovae we found, SN 2004am, shows rising X-ray flux for several years after explosion. There are only two supernovae, SN 1996cr and SN 1987A, which have similar long-term X-ray light curve. By comparing SN 2004am with SN 1996cr and SN 1987A, we might be able to gain valuable information about the circumstellar matter density structure. Hence, confirming the nature of SN 2004am will add an important sample in studying late-time behaviors of Type II supernovae. New follow-up Chandra observations would be useful to constrain the nature. Therefore, we present a proposed Chandra observation to monitor SN 2004am.

    § Chapter 1: Introduction 1 1.1 Brief History of X-rays from Nearby Galaxies 1 1.2 The Chandra X-ray Observatory 3 1.3 X-ray Emission of Nearby Galaxies 5 1.3.1 X-ray Binaries 5 1.3.2 Ultraluminous X-ray Sources 7 1.3.3 Supersoft X-ray Sources 8 1.3.4 Supernova Remnants 8 1.4 X-ray Source Population of Nearby Galaxies 8 1.4.1 The X-ray Luminosity Function 9 1.4.2 Source Distribution on X-ray Color-color Diagrams 9 1.5 X-ray Variability 11 1.6 Research Outline 14 § Chapter 2: Observations and Data Analysis 17 2.1 Observations 17 2.2 Data Reduction 18 2.3 Source Detection 19 2.4 Light Curves 20 2.5 Hardness Ratios 20 2.6 Variability 21 § Chapter 3: Results 23 3.1 Source Detection 23 3.2 Variability 24 3.3 Individual Sources 28 3.3.1 Transients 29 3.3.2 Spectral Variables 36 3.3.3 Supernova Remnants 38 § Chapter 4: A Proposed Chandra Study of the X-ray Evolution of Supernova 2004am 42 4.1 Introduction 42 4.2 X-ray Emission of Supernova Remnants 44 4.3 Target: SN 2004am 46 4.4 Proposed Chandra observation and feasibility 47 § Chapter 5: Discussion and Summary 50 5.1 Discussion 50 5.2 Summary 56 § Reference

    Aschenbach, B. 2002, Neutron Stars, Pulsars, and Supernova Remnants, 13

    Bauer, F. E., Dwarkadas, V. V., Brandt, W. N., Immler, S., Smartt, S., Bartel, N., & Bietenholz, M. F. 2008, ApJ, 688, 1210

    Beswick, R. J., Muxlow, T. W. B., Argo, M. K., & Pedlar, A. 2004, IAU Circ., 8332, 2

    Brandt, W. N., et al. 2001, AJ, 122, 2810

    Chandra Proposers’ Observatory Guide, POG

    Chevalier, R. A., & Fransson, C. 1992, ApJ, 395, 540

    Chevalier, R. A., & Fransson, C. 1994, ApJ, 420, 268

    Clemens, M. S., Alexander, P., & Green, D. A. 1999, mnras, 307, 481

    Colbert, E. J. M., & Mushotzky, R. F. 1999, Advances in Space Research, 23, 847

    Colbert, E. J. M., Heckman, T. M., Ptak, A. F., Strickland, D. K., & Weaver, K. A. 2004, apj, 602, 231

    Crosthwaite, L. P., & Turner, J. L. 2007, aj, 134, 1827

    Dewangan, G. C., Titarchuk, L., & Griffiths, R. E. 2006, apjl, 637, L21

    Di Stefano, R., & Kong, A. K. H. 2003, ApJ, 592, 884

    Esin, A. A., McClintock, J. E., & Narayan, R. 1997, ApJ, 489, 865

    Fabbiano, G. 1989, araa, 27, 87

    Fabbiano, G., & White, N. E. 2006, in Compact Stellar X-Ray Sources, ed. W. H. G. Lewin & M. van der Klis (Cambridge: Cambridge Univ. Press), 475

    Fabbiano, G. 2006, ARA&A, 44, 323

    Fender, R., & Maccarone, T. 2004, Cosmic Gamma-Ray Sources, 304, 205

    Fenech, D. M., Muxlow, T. W. B., Beswick, R. J., Pedlar, A., & Argo, M. K. 2008, MNRAS, 391, 1384

    Feng, H., & Kaaret, P. 2006, apj, 653, 536

    Freedman, W. L., et al. 1994, ApJ, 427, 628

    Fridriksson, J. K., Homan, J., Lewin, W. H. G., Kong, A. K. H., & Pooley, D. 2008, ApJS, 177, 465

    Gehrels, N. 1986, ApJ, 303, 336

    Georganopoulos, M., Aharonian, F. A., & Kirk, J. G. 2002, aap, 388, L25

    Greiner, J., Di Stefano, R., Kong, A., & Primini, F. 2004, apj, 610, 261

    Griffiths, R. E., Ptak, A., Feigelson, E. D., Garmire, G., Townsley, L., Brandt, W. N., Sambruna, R., & Bregman, J. N. 2000, Science, 290, 1325

    Grimm, H.J., Gilfanov, M., & Sunyaev, R. 2002, aap, 391, 923

    Grimm, H.-J., Gilfanov, M., & Sunyaev, R. 2003, mnras, 339, 793

    Hasinger, G., & van der Klis, M. 1989, aap, 225, 79

    Helfand, D. J., & Moran, E. C. 2001, ApJ, 554, 27

    Immler, S., & Lewin, W. H. G. 2003, Supernovae and Gamma-Ray Bursters, 598, 91

    Immler, S. et al. 2008, ApJ, 674, L85

    Irwin, J. A. 2006, mnras, 371, 1903

    Kaaret, P., Prestwich, A. H., Zezas, A., Murray, S. S., Kim, D.-W., Kilgard, R. E., Schlegel, E. M., & Ward, M. J. 2001, MNRAS, 321, L29

    Kilgard, R. E., Kaaret, P., Krauss, M. I., Prestwich, A. H., Raley, M. T., & Zezas, A. 2002, ApJ, 573, 138

    Kim, D.W., & Fabbiano, G. 2004, apj, 611, 846

    Kong, A. K. H., Garcia, M. R., Primini, F. A., Murray, S. S., Di Stefano, R., & McClintock, J. E. 2002, ApJ, 577, 738

    Kong, A. K. H., DiStefano, R., Garcia, M. R., & Greiner, J. 2003, apj, 585, 298

    Kong, A. K. H., Di Stefano, R., & Yuan, F. 2004, ApJ, 617, L49

    Kong, A. K. H., & Di Stefano, R. 2005, ApJ, 632, L107

    Kong, A. K. H., Yang, Y. J., Hsieh, P.-Y., Mak, D. S. Y., & Pun, C. S. J. 2007, ApJ, 671, 349

    Mattila, S., Meikle, W. P. S., Groeningsson, P., Greimel, R., Schirmer, M., Acosta-Pulido, J. A., & Li, W. 2004, IAU Circ., 8299, 2

    McDonald, A. R., Muxlow, T. W. B., Pedlar, A., Garrett, M. A., Wills, K. A., Garrington, S. T., Diamond, P. J., & Wilkinson, P. N. 2001, MNRAS, 322, 100

    Kahabka, P. 2002, arXiv:astro-ph/0212037

    Keto, E., Ho, L.C., & Lo, K.-Y. 2005, ApJ, 635, 1062

    Kilgard, R.E., Kaaret, P., Krauss, M.I., Prestwich, A.H., Raley, M.T., & Zezas, A. 2002, apj, 573, 138

    King, A. R., Davies, M. B., Ward, M. J., Fabbiano, G., & Elvis, M. 2001, apjl, 552, L109

    Kumagai, S., Shigeyama, T., Nomoto, K., Itoh, M., Nishimura, J., & Tsuruta, S. 1989, ApJ, 345, 412

    McClintock, J. E., & Remillard, R. A. 2003, arXiv:astro-ph/0306213

    McClintock, J. E., & Remillard, R. A. 2006, Compact stellar X-ray sources, 157

    McDonald, A. R., Muxlow, T. W. B., Wills, K. A., Pedlar, A., & Beswick, R. J. 2002, MNRAS, 334, 912

    Misanovic, Z., Pietsch, W., Haberl, F., Ehle, M., Hatzidimitriou, D., & Trinchieri, G. 2005, 5 years of Science with XMM-Newton, 99

    Muno, M. P., Remillard, R. A., & Chakrabarty, D. 2002, apjl, 568, L35

    Park, S., Zhekov, S. A., Burrows, D. N., Garmire, G. P., Racusin, J. L., & McCray, R. 2006, ApJ, 646, 1001

    Postnov, K.A. 2003, Astronomy Letters, 29, 372

    Prestwich, A. H., Irwin, J. A., Kilgard, R. E., Krauss, M. I., Zezas, A., Primini, F., Kaaret, P., & Boroson, B. 2003, ApJ, 595, 719

    Sauty, S., Gerin, M., & Casoli, F. 1998, aap, 339, 19

    Schulz, N. S., Hasinger, G., & Truemper, J. 1989, aap, 225, 48

    Singer, D., Pugh, H., & Li, W. 2004, IAU Circ., 8297, 2

    Sivakoff, G. R., Jord'an, A., Juett, A. M., Sarazin, C. L., & Irwin, J. A. 2008, arXiv:0806.0627

    Swartz, D. A., Ghosh, K. K., Tennant, A. F., & Wu, K. 2004, apjs, 154, 519

    van der Marel, R. P. 2004, Coevolution of Black Holes and Galaxies, 37

    van Paradijs, J. 1996, apjl, 464, L139

    Webbink, R.F. 2001, Evolution of Binary and Multiple Star Systems, 229, 309

    White, N. E. 1989, aapr, 1, 85

    Williams, B. F., Garcia, M. R., Kong, A. K. H., Primini, F. A., King, A. R., Di Stefano, R., & Murray, S. S. 2004, ApJ, 609, 735

    Wu, K. 2001, Publications of the Astronomical Society of Australia, 18, 443

    Zezas, A., Fabbiano, G., Prestwich, A., Murray, S., & Ward, M. 2001, The Central Kiloparsec of Starbursts and AGN: The La Palma Connection, 249, 425

    Zezas, A. 2006, Advances in Space Research, 38, 2946

    NASA/IPAC Extragalactic Database, http://nedwww.ipac.caltech.edu/

    無法下載圖示 全文公開日期 本全文未授權公開 (校內網路)
    全文公開日期 本全文未授權公開 (校外網路)

    QR CODE