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Searching for Binary and Dual Supermassive Black Holes in Large Surveys
Searching for Binary and Dual Supermassive Black Holes in Large Surveys
Searching for Binary and Dual Supermassive Black Holes in Large Surveys

상세정보

자료유형  
 학위논문 서양
최종처리일시  
20260202105211
ISBN  
9798291563946
DDC  
520
저자명  
Chen, Yu-Ching Tony.
서명/저자  
Searching for Binary and Dual Supermassive Black Holes in Large Surveys
발행사항  
[Sl] : University of Illinois at Urbana-Champaign, 2023
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2023
형태사항  
202 p
주기사항  
Source: Dissertations Abstracts International, Volume: 87-02, Section: B.
주기사항  
Advisor: Gammie, Charles;Liu, Xin.
학위논문주기  
Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2023.
초록/해제  
요약The observed structure of the universe suggests that galaxy mergers and the co-evolution of their central supermassive black holes (SMBHs) are common throughout the cosmos. While the formation of binary SMBHs seems inevitable, direct observational evidence of binary SMBHs has been elusive. No gravitational wave has yet been detected from the coalescence of a binary SMBH in the local universe. Evolution of binary SMBHs from kilo-parsec to sub-parsec scales and their interactions with host galaxies are still not well understood. Active SMBHs, known as quasars, provide an excellent way to study distant SMBHs in electromagnetic waves. A census of dual and binary quasars in different scales remains an essential puzzle in many aspects of astronomy. This dissertation consists of several studies aimed at searching for dual and binary quasars on different scales, from kilo-parsec to milliparsec. Chapter 2 focuses on discovering kilo-parsec dual quasar candidates using a novel astrometric technique. Chapter 3 presents a case study of a confirmed kilo-parsec dual quasar in a galaxy merger at a redshift of 2.17. In Chapter 4, the focus shifts to the search for dual/offset quasar candidates with parsec-scale separations. Chapter 5 presents a systematic search of periodic quasars, which are thought to be sub-parsec binary SMBHs, using optical light curves. Chapter 6 investigates the processing jet scenario for three periodic quasar candidates discovered in Chapter 5. This thesis paves the way for discovering dual and binary quasars using various methods and provides implications for future telescopes and surveys.
일반주제명  
Astronomy
일반주제명  
Astrophysics
일반주제명  
Aeronomy
키워드  
Active galaxies
키워드  
Quasars
키워드  
Binaries
키워드  
Galaxy evolution
키워드  
Surveys
기타저자  
University of Illinois at Urbana-Champaign Astronomy
기본자료저록  
Dissertations Abstracts International. 87-02B.
전자적 위치 및 접속  
로그인 후 원문을 볼 수 있습니다.

MARC

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■1001  ▼aChen,  Yu-Ching  Tony.
■24510▼aSearching  for  Binary  and  Dual  Supermassive  Black  Holes  in  Large  Surveys
■260    ▼a[Sl]▼bUniversity  of  Illinois  at  Urbana-Champaign▼c2023
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2023
■300    ▼a202  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  87-02,  Section:  B.
■500    ▼aAdvisor:  Gammie,  Charles;Liu,  Xin.
■5021  ▼aThesis  (Ph.D.)--University  of  Illinois  at  Urbana-Champaign,  2023.
■520    ▼aThe  observed  structure  of  the  universe  suggests  that  galaxy  mergers  and  the  co-evolution  of  their  central  supermassive  black  holes  (SMBHs)  are  common  throughout  the  cosmos.  While  the  formation  of  binary  SMBHs  seems  inevitable,  direct  observational  evidence  of  binary  SMBHs  has  been  elusive.  No  gravitational  wave  has  yet  been  detected  from  the  coalescence  of  a  binary  SMBH  in  the  local  universe.  Evolution  of  binary  SMBHs  from  kilo-parsec  to  sub-parsec  scales  and  their  interactions  with  host  galaxies  are  still  not  well  understood.  Active  SMBHs,  known  as  quasars,  provide  an  excellent  way  to  study  distant  SMBHs  in  electromagnetic  waves.  A  census  of  dual  and  binary  quasars  in  different  scales  remains  an  essential  puzzle  in  many  aspects  of  astronomy.  This  dissertation  consists  of  several  studies  aimed  at  searching  for  dual  and  binary  quasars  on  different  scales,  from  kilo-parsec  to  milliparsec.  Chapter  2  focuses  on  discovering  kilo-parsec  dual  quasar  candidates  using  a  novel  astrometric  technique.  Chapter  3  presents  a  case  study  of  a  confirmed  kilo-parsec  dual  quasar  in  a  galaxy  merger  at  a  redshift  of  2.17.  In  Chapter  4,  the  focus  shifts  to  the  search  for  dual/offset  quasar  candidates  with  parsec-scale  separations.  Chapter  5  presents  a  systematic  search  of  periodic  quasars,  which  are  thought  to  be  sub-parsec  binary  SMBHs,  using  optical  light  curves.  Chapter  6  investigates  the  processing  jet  scenario  for  three  periodic  quasar  candidates  discovered  in  Chapter  5.  This  thesis  paves  the  way  for  discovering  dual  and  binary  quasars  using  various  methods  and  provides  implications  for  future  telescopes  and  surveys.
■590    ▼aSchool  code:  0090.
■650  4▼aAstronomy
■650  4▼aAstrophysics
■650  4▼aAeronomy
■653    ▼aActive  galaxies
■653    ▼aQuasars
■653    ▼aBinaries
■653    ▼aGalaxy  evolution
■653    ▼aSurveys
■690    ▼a0606
■690    ▼a0367
■690    ▼a0596
■71020▼aUniversity  of  Illinois  at  Urbana-Champaign▼bAstronomy.
■7730  ▼tDissertations  Abstracts  International▼g87-02B.
■790    ▼a0090
■791    ▼aPh.D.
■792    ▼a2023
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17359771▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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