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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F14%3A00442418%21RIV15-AV0-67985815
rdf:type
n5:Vysledek skos:Concept
dcterms:description
Nuclear star clusters are unambiguously detected in about 50-70% of spiral and spheroidal galaxies. They have typical half-light radii of 2-5 pc, dynamical mass ranging from 106 - 107 M-circle, are brighter than globular clusters, and obey similar scaling relations with host galaxies as supermassive black holes. The nuclear stellar cluster (NSC) which surrounds Sgr A*, the SMBH at the center of our galaxy, is the nearest nuclear cluster to us, and can be resolved to scales of milliparsecs. The strong and highly variable extinction towards the Galactic center makes it very hard to infer the intrinsic properties of the NSC (structure and size). We attempt a new way to infer its properties by using Spitzer MIR images in a wavelength range 3-8 μm where the extinction is at a minimum, and the NSC clearly stands out as a separate structure. We present results from our analysis, including extinction-corrected images and surface brightness profiles of the central few hundred parsecs of the Milky Way. Nuclear star clusters are unambiguously detected in about 50-70% of spiral and spheroidal galaxies. They have typical half-light radii of 2-5 pc, dynamical mass ranging from 106 - 107 M-circle, are brighter than globular clusters, and obey similar scaling relations with host galaxies as supermassive black holes. The nuclear stellar cluster (NSC) which surrounds Sgr A*, the SMBH at the center of our galaxy, is the nearest nuclear cluster to us, and can be resolved to scales of milliparsecs. The strong and highly variable extinction towards the Galactic center makes it very hard to infer the intrinsic properties of the NSC (structure and size). We attempt a new way to infer its properties by using Spitzer MIR images in a wavelength range 3-8 μm where the extinction is at a minimum, and the NSC clearly stands out as a separate structure. We present results from our analysis, including extinction-corrected images and surface brightness profiles of the central few hundred parsecs of the Milky Way.
dcterms:title
Structure of the nuclear stellar cluster of the Milky Way galaxy Structure of the nuclear stellar cluster of the Milky Way galaxy
skos:prefLabel
Structure of the nuclear stellar cluster of the Milky Way galaxy Structure of the nuclear stellar cluster of the Milky Way galaxy
skos:notation
RIV/67985815:_____/14:00442418!RIV15-AV0-67985815
n3:aktivita
n16:I
n3:aktivity
I
n3:dodaniDat
n10:2015
n3:domaciTvurceVysledku
n15:5011833
n3:druhVysledku
n20:D
n3:duvernostUdaju
n11:S
n3:entitaPredkladatele
n13:predkladatel
n3:idSjednocenehoVysledku
47942
n3:idVysledku
RIV/67985815:_____/14:00442418
n3:jazykVysledku
n19:eng
n3:klicovaSlova
nuclear stellar cluster; Spitzer MIR images
n3:klicoveSlovo
n9:nuclear%20stellar%20cluster n9:Spitzer%20MIR%20images
n3:kontrolniKodProRIV
[94C7E96571B5]
n3:mistoKonaniAkce
Santa Fe
n3:mistoVydani
Cambridge
n3:nazevZdroje
The Galactic center: Feeding and Feedback in a Normal Galactic Nucleus
n3:obor
n14:BN
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
4
n3:rokUplatneniVysledku
n10:2014
n3:tvurceVysledku
Kunneriath, Devaky Stolovy, S. Schödel, R. Feldmeier, A.
n3:typAkce
n4:WRD
n3:zahajeniAkce
2013-09-30+02:00
s:issn
1743-9213
s:numberOfPages
2
n7:doi
10.1017/S1743921314000623
n18:hasPublisher
Cambridge University Press
n8:isbn
9781107044616