Obscuring and Feeding Supermassive Black Holes with Evolving Nuclear Star Clusters

Recently, high-resolution observations made with the help of the near-infrared adaptive optics integral field spectrograph SINFONI at the VLT proved the existence of massive and young nuclear star clusters in the centers of a sample of Seyfert galaxies. With the help of high-resolution hydrodynamica...

Celý popis

Uložené v:
Podrobná bibliografia
Vydané v:Proceedings of the International Astronomical Union Ročník 5; číslo S267; s. 307 - 312
Hlavní autori: Schartmann, M., Burkert, A., Krause, M., Camenzind, M., Meisenheimer, K., Davies, R. I.
Médium: Journal Article
Jazyk:English
Vydavateľské údaje: Cambridge, UK Cambridge University Press 01.08.2009
Predmet:
Astrophysics
Black holes
Contributed Papers
Fluid mechanics
Kinematics
Star & galaxy formation
Stars & galaxies
galaxies: Seyfert
galaxies: individual (NGC 1068)
black hole physics
ISM: evolution
galaxies: ISM
ISM: kinematics and dynamics
hydrodynamics
galaxies: nuclei
methods: numerical
stars: mass loss
ISSN:1743-9213, 1743-9221
On-line prístup:Získať plný text
Tagy: Pridať tag
Žiadne tagy, Buďte prvý, kto otaguje tento záznam!
Abstract Recently, high-resolution observations made with the help of the near-infrared adaptive optics integral field spectrograph SINFONI at the VLT proved the existence of massive and young nuclear star clusters in the centers of a sample of Seyfert galaxies. With the help of high-resolution hydrodynamical simulations with the pluto code, we follow the evolution of such clusters, especially focusing on mass and energy feedback from young stars. This leads to a filamentary inflow of gas on large scales (tens of parsecs), whereas a turbulent and very dense disk builds up on the parsec scale. Here we concentrate on the long-term evolution of the nuclear disk in NGC 1068 with the help of an effective viscous disk model, using the mass input from the large-scale simulations and accounting for star formation in the disk. This two-stage modeling enables us to connect the tens-of-parsecs scale region (observable with SINFONI) with the parsec-scale environment (MIDI observations). At the current age of the nuclear star cluster, our simulations predict disk sizes of the order 0.8 to 0.9 pc, gas masses of order 106M⊙, and mass transfer rates through the inner boundary of order 0.025 M⊙yr−1, in good agreement with values derived from observations.
AbstractList Recently, high-resolution observations made with the help of the near-infrared adaptive optics integral field spectrograph SINFONI at the VLT proved the existence of massive and young nuclear star clusters in the centers of a sample of Seyfert galaxies. With the help of high-resolution hydrodynamical simulations with the pluto code, we follow the evolution of such clusters, especially focusing on mass and energy feedback from young stars. This leads to a filamentary inflow of gas on large scales (tens of parsecs), whereas a turbulent and very dense disk builds up on the parsec scale. Here we concentrate on the long-term evolution of the nuclear disk in NGC 1068 with the help of an effective viscous disk model, using the mass input from the large-scale simulations and accounting for star formation in the disk. This two-stage modeling enables us to connect the tens-of-parsecs scale region (observable with SINFONI) with the parsec-scale environment (MIDI observations). At the current age of the nuclear star cluster, our simulations predict disk sizes of the order 0.8 to 0.9 pc, gas masses of order 106 M[odot], and mass transfer rates through the inner boundary of order 0.025 M[odot] yr-1, in good agreement with values derived from observations.
Recently, high-resolution observations made with the help of the near-infrared adaptive optics integral field spectrograph SINFONI at the VLT proved the existence of massive and young nuclear star clusters in the centers of a sample of Seyfert galaxies. With the help of high-resolution hydrodynamical simulations with the pluto code, we follow the evolution of such clusters, especially focusing on mass and energy feedback from young stars. This leads to a filamentary inflow of gas on large scales (tens of parsecs), whereas a turbulent and very dense disk builds up on the parsec scale. Here we concentrate on the long-term evolution of the nuclear disk in NGC 1068 with the help of an effective viscous disk model, using the mass input from the large-scale simulations and accounting for star formation in the disk. This two-stage modeling enables us to connect the tens-of-parsecs scale region (observable with SINFONI) with the parsec-scale environment (MIDI observations). At the current age of the nuclear star cluster, our simulations predict disk sizes of the order 0.8 to 0.9 pc, gas masses of order 106M⊙, and mass transfer rates through the inner boundary of order 0.025 M⊙yr−1, in good agreement with values derived from observations.
Recently, high-resolution observations made with the help of the near-infrared adaptive optics integral field spectrograph SINFONI at the VLT proved the existence of massive and young nuclear star clusters in the centers of a sample of Seyfert galaxies. With the help of high-resolution hydrodynamical simulations with the pluto code, we follow the evolution of such clusters, especially focusing on mass and energy feedback from young stars. This leads to a filamentary inflow of gas on large scales (tens of parsecs), whereas a turbulent and very dense disk builds up on the parsec scale. Here we concentrate on the long-term evolution of the nuclear disk in NGC 1068 with the help of an effective viscous disk model, using the mass input from the large-scale simulations and accounting for star formation in the disk. This two-stage modeling enables us to connect the tens-of-parsecs scale region (observable with SINFONI) with the parsec-scale environment (MIDI observations). At the current age of the nuclear star cluster, our simulations predict disk sizes of the order 0.8 to 0.9 pc, gas masses of order 106 M[middot in circle], and mass transfer rates through the inner boundary of order 0.025 M[middot in circle] yr-1, in good agreement with values derived from observations. [PUBLICATION ABSTRACT]
Recently, high-resolution observations made with the help of the near-infrared adaptive optics integral field spectrograph SINFONI at the VLT proved the existence of massive and young nuclear star clusters in the centers of a sample of Seyfert galaxies. With the help of high-resolution hydrodynamical simulations with the pluto code, we follow the evolution of such clusters, especially focusing on mass and energy feedback from young stars. This leads to a filamentary inflow of gas on large scales (tens of parsecs), whereas a turbulent and very dense disk builds up on the parsec scale. Here we concentrate on the long-term evolution of the nuclear disk in NGC 1068 with the help of an effective viscous disk model, using the mass input from the large-scale simulations and accounting for star formation in the disk. This two-stage modeling enables us to connect the tens-of-parsecs scale region (observable with SINFONI) with the parsec-scale environment (MIDI observations). At the current age of the nuclear star cluster, our simulations predict disk sizes of the order 0.8 to 0.9 pc, gas masses of order 10 6 M ⊙ , and mass transfer rates through the inner boundary of order 0.025 M ⊙ yr −1 , in good agreement with values derived from observations.
Author Davies, R. I.
Krause, M.
Meisenheimer, K.
Schartmann, M.
Camenzind, M.
Burkert, A.
Author_xml – sequence: 1
  givenname: M.
  surname: Schartmann
  fullname: Schartmann, M.
  email: schartmann@mpe.mpg.de
  organization: 1Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching, Germany Email: schartmann@mpe.mpg.de
– sequence: 2
  givenname: A.
  surname: Burkert
  fullname: Burkert, A.
  email: schartmann@mpe.mpg.de
  organization: 1Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching, Germany Email: schartmann@mpe.mpg.de
– sequence: 3
  givenname: M.
  surname: Krause
  fullname: Krause, M.
  email: schartmann@mpe.mpg.de
  organization: 1Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching, Germany Email: schartmann@mpe.mpg.de
– sequence: 4
  givenname: M.
  surname: Camenzind
  fullname: Camenzind, M.
  organization: 4ZAH – Landessternwarte Heidelberg, Königstuhl 12, 69117 Heidelberg, Germany
– sequence: 5
  givenname: K.
  surname: Meisenheimer
  fullname: Meisenheimer, K.
  organization: 5Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
– sequence: 6
  givenname: R. I.
  surname: Davies
  fullname: Davies, R. I.
  email: schartmann@mpe.mpg.de
  organization: 1Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, 85748 Garching, Germany Email: schartmann@mpe.mpg.de
BookMark eNp1kE1Lw0AQhhepYFv9Ad6CF0_V_cpuc9TSWqFYsHoO-zGpqZuk7iYV_72JLQqKl5lheN6XmXeAemVVAkLnBF8RTOT1ikjOEkoYwRiLmIoj1O9Wo4RS0vueCTtBgxA2GHMxZnEfPS51MI3Py3WkShvNAGw3r5ot-EKFkO8gunXKvEbzykGI3vP6JZruKrfrsIfGOFA-WtVtmbgm1ODDKTrOlAtwduhD9DybPk3mo8Xy7n5ysxgZxlk9UlZnWtMYG62SjFgpMLWSk4zFhsDYCJ1QCZxzyTBJDAdQ2rIWARtbmlk2RJd7362v3hoIdVrkwYBzqoSqCankseCs_bQlL36Rm6rxZXtcyoSQCeFfENlDxlcheMjSrc8L5T9SgtMu4_RPxq2GHTSq0D63a_hx_l_1CXu9f8M
Cites_doi 10.1088/0004-637X/705/1/L53
10.1086/523032
10.1111/j.1365-2966.2008.14220.x
10.1086/184981
10.1038/nature02531
10.1111/j.1365-2966.2009.14439.x
10.1146/annurev.aa.19.090181.001033
10.1007/3-540-34621-X_6
10.1086/307375
ContentType Journal Article
Copyright Copyright © International Astronomical Union 2010
Copyright_xml – notice: Copyright © International Astronomical Union 2010
DBID AAYXX
CITATION
3V.
7XB
88I
8FD
8FE
8FG
8FK
ABUWG
AFKRA
ARAPS
AZQEC
BENPR
BGLVJ
CCPQU
DWQXO
GNUQQ
H8D
HCIFZ
L7M
M2P
P5Z
P62
PHGZM
PHGZT
PKEHL
PQEST
PQGLB
PQQKQ
PQUKI
PRINS
Q9U
7TG
KL.
DOI 10.1017/S1743921310006526
DatabaseName CrossRef
ProQuest Central (Corporate)
ProQuest Central (purchase pre-March 2016)
Science Database (Alumni Edition)
Technology Research Database
ProQuest SciTech Collection
ProQuest Technology Collection
ProQuest Central (Alumni) (purchase pre-March 2016)
ProQuest Central (Alumni)
ProQuest Central UK/Ireland
ProQuest Advanced Technologies & Aerospace Collection
ProQuest Central Essentials
ProQuest Central
Technology collection
ProQuest One Community College
ProQuest Central
ProQuest Central Student
Aerospace Database
SciTech Premium Collection
Advanced Technologies Database with Aerospace
Science Database
Advanced Technologies & Aerospace Database
ProQuest Advanced Technologies & Aerospace Collection
ProQuest Central Premium
ProQuest One Academic
ProQuest One Academic Middle East (New)
ProQuest One Academic Eastern Edition (DO NOT USE)
ProQuest One Applied & Life Sciences
ProQuest One Academic (retired)
ProQuest One Academic UKI Edition
ProQuest Central China
ProQuest Central Basic
Meteorological & Geoastrophysical Abstracts
Meteorological & Geoastrophysical Abstracts - Academic
DatabaseTitle CrossRef
ProQuest Central Student
Technology Collection
Technology Research Database
ProQuest One Academic Middle East (New)
ProQuest Advanced Technologies & Aerospace Collection
ProQuest Central Essentials
ProQuest Central (Alumni Edition)
SciTech Premium Collection
ProQuest One Community College
ProQuest Central China
ProQuest Central
ProQuest One Applied & Life Sciences
Aerospace Database
ProQuest Central Korea
ProQuest Central (New)
Advanced Technologies Database with Aerospace
Advanced Technologies & Aerospace Collection
ProQuest Science Journals (Alumni Edition)
ProQuest Central Basic
ProQuest Science Journals
ProQuest One Academic Eastern Edition
ProQuest Technology Collection
ProQuest SciTech Collection
Advanced Technologies & Aerospace Database
ProQuest One Academic UKI Edition
ProQuest One Academic
ProQuest Central (Alumni)
ProQuest One Academic (New)
Meteorological & Geoastrophysical Abstracts - Academic
Meteorological & Geoastrophysical Abstracts
DatabaseTitleList Meteorological & Geoastrophysical Abstracts - Academic

ProQuest Central Student
CrossRef
Database_xml – sequence: 1
  dbid: BENPR
  name: ProQuest Central
  url: https://www.proquest.com/central
  sourceTypes: Aggregation Database
DeliveryMethod fulltext_linktorsrc
Discipline Astronomy & Astrophysics
EISSN 1743-9221
EndPage 312
ExternalDocumentID 2055770631
10_1017_S1743921310006526
Genre Feature
GroupedDBID -E.
.FH
09C
09E
0E1
0R~
123
29P
3V.
4.4
5VS
74X
74Y
7~V
88I
8FE
8FG
8FH
8R4
8R5
AAAZR
AABES
AABWE
AACJH
AAGFV
AAKTX
AANRG
AARAB
AASVR
AAUKB
ABBXD
ABBZL
ABDBF
ABGDZ
ABITZ
ABJNI
ABKKG
ABMWE
ABQTM
ABROB
ABUWG
ABVKB
ABVZP
ABXAU
ABZCX
ACBMC
ACDLN
ACGFS
ACGOD
ACIMK
ACQPF
ACUHS
ACUIJ
ACYZP
ACZBM
ACZUX
ACZWT
ADCGK
ADDNB
ADFEC
ADKIL
ADOVH
ADOVT
ADVJH
AEBAK
AEHGV
AEMTW
AENCP
AENGE
AEYYC
AFFUJ
AFKQG
AFKRA
AFLOS
AFLVW
AFUTZ
AFZFC
AGABE
AGBYD
AGJUD
AHQXX
AHRGI
AIGNW
AIHIV
AIOIP
AISIE
AJ7
AJCYY
AJPFC
AJQAS
AKZCZ
ALMA_UNASSIGNED_HOLDINGS
ALVPG
ALWZO
AQJOH
ARABE
ARAPS
ARZZG
ATUCA
AUXHV
AYIQA
AZQEC
BBLKV
BCGOX
BENPR
BESQT
BGHMG
BGLVJ
BJBOZ
BLZWO
BMAJL
BPHCQ
C0O
CAG
CBIIA
CCPQU
CCQAD
CCUQV
CFAFE
CFBFF
CGQII
CHEAL
CJCSC
COF
CS3
D1K
DC4
DOHLZ
DWQXO
EBS
EGQIC
EJD
GNUQQ
HCIFZ
HG-
HST
HZ~
I.6
IH6
IOEEP
IOO
IS6
I~P
J36
J38
J3A
JHPGK
JQKCU
K6-
KAFGG
KCGVB
KFECR
L98
LHUNA
LK5
LW7
M-V
M2P
M7R
NIKVX
NZEOI
O9-
P62
PQQKQ
PROAC
PYCCK
Q2X
RAMDC
RCA
ROL
RR0
S6-
S6U
SAAAG
T9M
UT1
WFFJZ
WQ3
WXU
WYP
ZDLDU
ZJOSE
ZMEZD
ZYDXJ
AAXMD
AAYXX
ABXHF
AFFHD
AKMAY
CITATION
PHGZM
PHGZT
PQGLB
7XB
8FD
8FK
H8D
L7M
PKEHL
PQEST
PQUKI
PRINS
Q9U
7TG
KL.
PUEGO
ID FETCH-LOGICAL-c343t-adbfbb250cba9f1d7602d741f35c1e8c6b927e44473019c4eeabd32d7ed5d2fd3
IEDL.DBID BENPR
ISICitedReferencesCount 0
ISICitedReferencesURI http://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=Summon&SrcAuth=ProQuest&DestLinkType=CitingArticles&DestApp=WOS_CPL&KeyUT=000291672300103&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D
ISSN 1743-9213
IngestDate Thu Oct 02 06:22:11 EDT 2025
Fri Jul 25 08:46:44 EDT 2025
Sat Nov 29 01:38:50 EST 2025
Tue Jan 21 06:24:29 EST 2025
IsDoiOpenAccess false
IsOpenAccess true
IsPeerReviewed true
IsScholarly true
Issue S267
Keywords galaxies: Seyfert
galaxies: individual (NGC 1068)
black hole physics
ISM: evolution
galaxies: ISM
ISM: kinematics and dynamics
hydrodynamics
galaxies: nuclei
methods: numerical
stars: mass loss
Language English
License https://www.cambridge.org/core/terms
LinkModel DirectLink
MergedId FETCHMERGED-LOGICAL-c343t-adbfbb250cba9f1d7602d741f35c1e8c6b927e44473019c4eeabd32d7ed5d2fd3
Notes SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 14
ObjectType-Article-2
content type line 23
OpenAccessLink https://www.cambridge.org/core/services/aop-cambridge-core/content/view/16C8406DADF553B20556D9A93EBA03C6/S1743921310006526a.pdf/div-class-title-obscuring-and-feeding-supermassive-black-holes-with-evolving-nuclear-star-clusters-div.pdf
PQID 366791404
PQPubID 39246
PageCount 6
ParticipantIDs proquest_miscellaneous_745643004
proquest_journals_366791404
crossref_primary_10_1017_S1743921310006526
cambridge_journals_10_1017_S1743921310006526
PublicationCentury 2000
PublicationDate 2009-08-00
PublicationDateYYYYMMDD 2009-08-01
PublicationDate_xml – month: 08
  year: 2009
  text: 2009-08-00
PublicationDecade 2000
PublicationPlace Cambridge, UK
PublicationPlace_xml – name: Cambridge, UK
– name: Cambridge
PublicationTitle Proceedings of the International Astronomical Union
PublicationTitleAlternate Proc. IAU
PublicationYear 2009
Publisher Cambridge University Press
Publisher_xml – name: Cambridge University Press
References S1743921310006526_ref9
S1743921310006526_ref11
S1743921310006526_ref13
Tristram (S1743921310006526_ref15) 2009; 502
S1743921310006526_ref12
Tristram (S1743921310006526_ref14) 2007; 474
Jungwiert (S1743921310006526_ref6) 2001; 376
Lodato (S1743921310006526_ref10) 2003; 398
S1743921310006526_ref8
S1743921310006526_ref5
Gallimore (S1743921310006526_ref3) 2003
S1743921310006526_ref4
Kishimoto (S1743921310006526_ref7) 2009; 493
S1743921310006526_ref1
S1743921310006526_ref2
References_xml – volume: 398
  start-page: 517
  year: 2003
  ident: S1743921310006526_ref10
  publication-title: AandA
– volume: 376
  start-page: 85
  year: 2001
  ident: S1743921310006526_ref6
  publication-title: AandA
– volume: 502
  start-page: 67
  year: 2009
  ident: S1743921310006526_ref15
  publication-title: AandA
– ident: S1743921310006526_ref1
  doi: 10.1088/0004-637X/705/1/L53
– ident: S1743921310006526_ref2
  doi: 10.1086/523032
– ident: S1743921310006526_ref13
  doi: 10.1111/j.1365-2966.2008.14220.x
– volume: 493
  start-page: L57
  year: 2009
  ident: S1743921310006526_ref7
  publication-title: AandA
– ident: S1743921310006526_ref9
  doi: 10.1086/184981
– ident: S1743921310006526_ref4
  doi: 10.1038/nature02531
– ident: S1743921310006526_ref12
  doi: 10.1111/j.1365-2966.2009.14439.x
– start-page: 501
  volume-title: Active Galactic Nuclei: From Central Engine to Host Galaxy
  year: 2003
  ident: S1743921310006526_ref3
– ident: S1743921310006526_ref11
  doi: 10.1146/annurev.aa.19.090181.001033
– volume: 474
  start-page: 837
  year: 2007
  ident: S1743921310006526_ref14
  publication-title: AandA
– ident: S1743921310006526_ref5
  doi: 10.1007/3-540-34621-X_6
– ident: S1743921310006526_ref8
  doi: 10.1086/307375
SSID ssj0046835
Score 1.7294835
Snippet Recently, high-resolution observations made with the help of the near-infrared adaptive optics integral field spectrograph SINFONI at the VLT proved the...
SourceID proquest
crossref
cambridge
SourceType Aggregation Database
Index Database
Publisher
StartPage 307
SubjectTerms Astrophysics
Black holes
Contributed Papers
Fluid mechanics
Kinematics
Star & galaxy formation
Stars & galaxies
Title Obscuring and Feeding Supermassive Black Holes with Evolving Nuclear Star Clusters
URI https://www.cambridge.org/core/product/identifier/S1743921310006526/type/journal_article
https://www.proquest.com/docview/366791404
https://www.proquest.com/docview/745643004
Volume 5
WOSCitedRecordID wos000291672300103&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D
hasFullText 1
inHoldings 1
isFullTextHit
isPrint
journalDatabaseRights – providerCode: PRVPQU
  databaseName: Advanced Technologies & Aerospace Database
  customDbUrl:
  eissn: 1743-9221
  dateEnd: 20241207
  omitProxy: false
  ssIdentifier: ssj0046835
  issn: 1743-9213
  databaseCode: P5Z
  dateStart: 20040301
  isFulltext: true
  titleUrlDefault: https://search.proquest.com/hightechjournals
  providerName: ProQuest
– providerCode: PRVPQU
  databaseName: ProQuest Central
  customDbUrl:
  eissn: 1743-9221
  dateEnd: 20241207
  omitProxy: false
  ssIdentifier: ssj0046835
  issn: 1743-9213
  databaseCode: BENPR
  dateStart: 20040301
  isFulltext: true
  titleUrlDefault: https://www.proquest.com/central
  providerName: ProQuest
– providerCode: PRVPQU
  databaseName: Science Database
  customDbUrl:
  eissn: 1743-9221
  dateEnd: 20241207
  omitProxy: false
  ssIdentifier: ssj0046835
  issn: 1743-9213
  databaseCode: M2P
  dateStart: 20040301
  isFulltext: true
  titleUrlDefault: https://search.proquest.com/sciencejournals
  providerName: ProQuest
link http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV1LS8NAEB60evDiW6yPsgfxIC6a7GbTnKRKiwetxQeIl5DsbEDQtDat4L93Z5NUiuDFSwjJsoTM7jdfZibfABypLDJCR-ccVYZcogh5Kn2PG99ou6DI6E5n9ibs99vPz9Ggqs0pqrLKGhMdUONQU4z8TCgVRqQFczH64NQ0ipKrVQeNRVgioTLZgKXLbn9wX0OxVG3XYZNYN498T9RpTdKMdlTcXvOcG54XV5h3UvMY7RxPb-2fj7wOqxXjZJ1yiWzAgsk3YbdTUAx8-P7Fjpk7L0McxRbc31kocT8vsiRH1ivdG3uYjgjECyp3Zy7sx65JDIpRJJd1LcpRaIL1SR85GTNLYsfs6m1KOgzFNjz1uo9X17zqvMC1kGLCE0yzNLXsSKdJlHkYqnMfLffIRKA909YqjfzQSCkJHyItjUlSFHaIwQD9DMUONPJhbnaBedpkmeenCQahlKjKrxSpNKJlOxg04XT22uNq_xRxWXsWxr-s1IST2jLxqNTj-Gvwfm2Yn6lnVmkCm921e4oSJUluhtMiDkljh6TI9v6cYB9WytwSlQMeQGMynppDWNafk9di3KrWYgsWb_2BPQ6Cl28izucn
linkProvider ProQuest
linkToHtml http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMw1V1NT-MwEB3xsRJcgGVBlE8flj0gLIjtOs1hhRBLVUTpooWVuIXE40hIkJamBfGj-I_rcZquKiRuHLhFSWQp8fO88cz4DcB3nUVWmuiQo86QK5QhT5UIuBXWOEDRpHud2XbY6TRubqLLKXitzsJQWWVlE72hxq6hGPmB1DqMSAvmqPfIqWkUJVerDholKs7ty7PbsRU_z3656d0Vonl6fdLio6YC3EglBzzBNEtTR_wmTaIswFAfCnS0msm6CWzD6DQSoVVKEfQjo6xNUpTuFYt1FBlKN-40zCq3EaJldSEuK8OvdMP38yQfn0cikFUSlRSqvePv7gWe9CelHCYpcZIRPM01Fz_ZD1qChZE_zY7LBfAVpmy-DGvHBUX4uw8v7Afz12UAp_gGf347Q-mPZrIkR9YsyZtdDXtEUQUV8zMf1GQtkrpiFKdmp86GU-CFdUj9Oekz56L32cn9kFQmihX4-yFfuAozeTe3a8ACY7MsEGmC9VAp1OUeTGmD6Hw5rNdgfzzN8cg6FHFZWRfGb1BRg70KCXGvVBt57-WNCgj_hx6joAZs_NRZDEoDJbntDos4JAUhElpbf3eAHZhrXV-04_ZZ53wD5sssGhU-bsLMoD-0W_DFPA3uiv62XwUMbj8aVf8ACWlDvw
openUrl ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Obscuring+and+Feeding+Supermassive+Black+Holes+with+Evolving+Nuclear+Star+Clusters&rft.jtitle=Proceedings+of+the+International+Astronomical+Union&rft.au=Schartmann%2C+M.&rft.au=Burkert%2C+A.&rft.au=Krause%2C+M.&rft.au=Camenzind%2C+M.&rft.date=2009-08-01&rft.issn=1743-9213&rft.eissn=1743-9221&rft.volume=5&rft.issue=S267&rft.spage=307&rft.epage=312&rft_id=info:doi/10.1017%2FS1743921310006526&rft.externalDBID=n%2Fa&rft.externalDocID=10_1017_S1743921310006526
thumbnail_l http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=1743-9213&client=summon
thumbnail_m http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=1743-9213&client=summon
thumbnail_s http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=1743-9213&client=summon