FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100687004> ?p ?o ?g. }

• W3100687004 endingPage "A156" @default.
• W3100687004 startingPage "A156" @default.
• W3100687004 abstract "Polar ring galaxies (PRGs) are composed of two kinematically distinct and nearly orthogonal components, a host galaxy (HG) and a polar ring/disk (PR). The HG usually contains an older stellar population than the PR. The suggested formation channel of PRGs is still poorly constrained. Suggested options are merger, gas accretion, tidal interaction, or a combination of both. To constrain the formation scenario of PRGs, we study the compact stellar systems (CSSs) in two PRGs at different evolutionary stages: NGC 4650A with well-defined PR, and NGC 3808B, which is in the process of PR formation. We use archival HST/WFPC2 imaging. PSF-fitting techniques, and color selection criteria are used to select cluster candidates. Photometric analysis of the CSSs was performed to determine their ages and masses using stellar population models at a fixed metallicity. Both PRGs contain young CSSs ($< 1$ Gyr) with masses of up to 5$times$10$^6$M$_odot$, mostly located in the PR and along the tidal debris. The most massive CSSs may be progenitors of metal-rich globular clusters or ultra compact dwarf (UCD) galaxies. We identify one such young UCD candidate, NGC 3808 B-8, and measure its size of $r_{rm eff}=25.23^{+1.43}_{-2.01}$ pc. We reconstruct the star formation history of the two PRGs and find strong peaks in the star formation rate (SFR $simeq$ 200M$_odot$/yr) in NGC 3808B, while NGC 4650A shows milder (declining) star formation (SFR $<$ 10M$_odot$/yr). This difference may support different evolutionary paths between these PRGs. The spatial distribution, masses, and peak star formation epoch of the clusters in NGC 3808 suggest for a tidally triggered star formation. Incompleteness at old ages prevents us from probing the SFR at earlier epochs of NGC 4650A, where we observe the fading tail of CSS formation. This also impedes us from testing the formation scenarios of this PRG." @default.
• W3100687004 created "2020-11-23" @default.
• W3100687004 creator A5016766986 @default.
• W3100687004 creator A5030400654 @default.
• W3100687004 creator A5039870273 @default.
• W3100687004 creator A5044934501 @default.
• W3100687004 creator A5085774111 @default.
• W3100687004 date "2016-01-01" @default.
• W3100687004 modified "2023-10-12" @default.
• W3100687004 title "Compact stellar systems in the polar ring galaxies NGC 4650A and NGC 3808B: Clues to polar disk formation" @default.
• W3100687004 cites W1484204443 @default.
• W3100687004 cites W1659678786 @default.
• W3100687004 cites W1977731007 @default.
• W3100687004 cites W1983266276 @default.
• W3100687004 cites W1990934390 @default.
• W3100687004 cites W1994421189 @default.
• W3100687004 cites W1994671833 @default.
• W3100687004 cites W1994998266 @default.
• W3100687004 cites W2007088574 @default.
• W3100687004 cites W2010491283 @default.
• W3100687004 cites W2015091650 @default.
• W3100687004 cites W2018078466 @default.
• W3100687004 cites W2021620550 @default.
• W3100687004 cites W2022489355 @default.
• W3100687004 cites W2029343094 @default.
• W3100687004 cites W2032750751 @default.
• W3100687004 cites W2041869266 @default.
• W3100687004 cites W2048756914 @default.
• W3100687004 cites W2049314947 @default.
• W3100687004 cites W2066034174 @default.
• W3100687004 cites W2069835397 @default.
• W3100687004 cites W2070762163 @default.
• W3100687004 cites W2085793384 @default.
• W3100687004 cites W2091141621 @default.
• W3100687004 cites W2093769398 @default.
• W3100687004 cites W2100833883 @default.
• W3100687004 cites W2107337450 @default.
• W3100687004 cites W2111767615 @default.
• W3100687004 cites W2111817932 @default.
• W3100687004 cites W2114368492 @default.
• W3100687004 cites W2124181276 @default.
• W3100687004 cites W2129760210 @default.
• W3100687004 cites W2142840856 @default.
• W3100687004 cites W2151008117 @default.
• W3100687004 cites W2161997838 @default.
• W3100687004 cites W2178336115 @default.
• W3100687004 cites W2952538582 @default.
• W3100687004 cites W3006237505 @default.
• W3100687004 cites W3099155372 @default.
• W3100687004 cites W3099484866 @default.
• W3100687004 cites W3099853403 @default.
• W3100687004 cites W3100910145 @default.
• W3100687004 cites W3100942935 @default.
• W3100687004 cites W3101266944 @default.
• W3100687004 cites W3101933151 @default.
• W3100687004 cites W3103692932 @default.
• W3100687004 cites W3103868583 @default.
• W3100687004 cites W3104079859 @default.
• W3100687004 cites W3104263850 @default.
• W3100687004 cites W3104592142 @default.
• W3100687004 cites W3104826024 @default.
• W3100687004 cites W3105565697 @default.
• W3100687004 cites W3106135675 @default.
• W3100687004 cites W3106265194 @default.
• W3100687004 cites W3106309143 @default.
• W3100687004 cites W3121591693 @default.
• W3100687004 cites W3122012004 @default.
• W3100687004 cites W3124405344 @default.
• W3100687004 cites W3125356176 @default.
• W3100687004 cites W4231802503 @default.
• W3100687004 cites W4290707612 @default.
• W3100687004 cites W4292480926 @default.
• W3100687004 cites W4298037686 @default.
• W3100687004 cites W4301685910 @default.
• W3100687004 cites W4302071094 @default.
• W3100687004 cites W79829610 @default.
• W3100687004 doi "https://doi.org/10.1051/0004-6361/201527025" @default.
• W3100687004 hasPublicationYear "2016" @default.
• W3100687004 type Work @default.
• W3100687004 sameAs 3100687004 @default.
• W3100687004 citedByCount "3" @default.
• W3100687004 countsByYear W31006870042017 @default.
• W3100687004 countsByYear W31006870042020 @default.
• W3100687004 countsByYear W31006870042022 @default.
• W3100687004 crossrefType "journal-article" @default.
• W3100687004 hasAuthorship W3100687004A5016766986 @default.
• W3100687004 hasAuthorship W3100687004A5030400654 @default.
• W3100687004 hasAuthorship W3100687004A5039870273 @default.
• W3100687004 hasAuthorship W3100687004A5044934501 @default.
• W3100687004 hasAuthorship W3100687004A5085774111 @default.
• W3100687004 hasBestOaLocation W31006870042 @default.
• W3100687004 hasConcept C113461152 @default.
• W3100687004 hasConcept C121332964 @default.
• W3100687004 hasConcept C125857072 @default.
• W3100687004 hasConcept C1276947 @default.
• W3100687004 hasConcept C144024400 @default.
• W3100687004 hasConcept C149923435 @default.
• W3100687004 hasConcept C2776401274 @default.

• next