Matches in SemOpenAlex for { <https://semopenalex.org/work/W2137467237> ?p ?o ?g. }
- W2137467237 endingPage "472" @default.
- W2137467237 startingPage "461" @default.
- W2137467237 abstract "We present sensitive ISO m observations of the edge-on galaxy, NGC 5529, finding an extensive MIR halo around NGC 5529. The emission is dominated by PAHs in this band. The PAH halo has an exponential scale height of 3.7 kpc but can still be detected as far as ≈10 kpc from the plane to the limits of the high dynamic range (1770/1) data. This is the most extensive PAH halo yet detected in a normal galaxy. This halo shows substructure and the PAHs likely originate from some type of disk outflow. PAHs are long-lived in a halo environment and therefore continuous replenishment from the disk is not required (unless halo PAHs are also being destroyed or removed), consistent with the current low SFR of the galaxy. The PAHs correlate spatially with halo Hα emission, previously observed by Miller & Veilleux (2003, ApJS, 148, 383); both components are likely excited/ionized by in-disk photons that are leaking into the halo. The presence of halo gas may be related to the environment of NGC 5529 which contains at least 17 galaxies in a small group of which NGC 5529 is the dominant member. Of these, we have identified two new companions from the SDSS." @default.
- W2137467237 created "2016-06-24" @default.
- W2137467237 creator A5003745554 @default.
- W2137467237 creator A5051687465 @default.
- W2137467237 creator A5081981032 @default.
- W2137467237 creator A5086494315 @default.
- W2137467237 date "2007-08-28" @default.
- W2137467237 modified "2023-09-27" @default.
- W2137467237 title "PAHs in the halo of NGC 5529" @default.
- W2137467237 cites W1628582679 @default.
- W2137467237 cites W1977890251 @default.
- W2137467237 cites W1982511713 @default.
- W2137467237 cites W1999767576 @default.
- W2137467237 cites W2003637061 @default.
- W2137467237 cites W2017055895 @default.
- W2137467237 cites W2033659194 @default.
- W2137467237 cites W2040721633 @default.
- W2137467237 cites W2042765983 @default.
- W2137467237 cites W2045869342 @default.
- W2137467237 cites W2047959841 @default.
- W2137467237 cites W2048274049 @default.
- W2137467237 cites W2048760245 @default.
- W2137467237 cites W2051068238 @default.
- W2137467237 cites W2059086184 @default.
- W2137467237 cites W2071700822 @default.
- W2137467237 cites W2084981136 @default.
- W2137467237 cites W2086235133 @default.
- W2137467237 cites W2115652448 @default.
- W2137467237 cites W2116466430 @default.
- W2137467237 cites W2121283100 @default.
- W2137467237 cites W2131303567 @default.
- W2137467237 cites W2131617810 @default.
- W2137467237 cites W2133069926 @default.
- W2137467237 cites W2138911062 @default.
- W2137467237 cites W2156387155 @default.
- W2137467237 cites W2156880259 @default.
- W2137467237 cites W2159987586 @default.
- W2137467237 cites W2160103415 @default.
- W2137467237 cites W2162124571 @default.
- W2137467237 cites W2163069091 @default.
- W2137467237 cites W2168495929 @default.
- W2137467237 cites W2170066079 @default.
- W2137467237 cites W2597722942 @default.
- W2137467237 cites W2600822636 @default.
- W2137467237 cites W2989273194 @default.
- W2137467237 cites W3100059901 @default.
- W2137467237 cites W3100416241 @default.
- W2137467237 cites W3101987177 @default.
- W2137467237 cites W3102027531 @default.
- W2137467237 cites W3102222087 @default.
- W2137467237 cites W3102277364 @default.
- W2137467237 cites W3102560695 @default.
- W2137467237 cites W3103914037 @default.
- W2137467237 cites W3104416848 @default.
- W2137467237 cites W3104986614 @default.
- W2137467237 cites W3105449104 @default.
- W2137467237 cites W3105543072 @default.
- W2137467237 cites W3105901391 @default.
- W2137467237 cites W3125905236 @default.
- W2137467237 cites W4245952677 @default.
- W2137467237 cites W4298872669 @default.
- W2137467237 cites W4301519098 @default.
- W2137467237 doi "https://doi.org/10.1051/0004-6361:20077729" @default.
- W2137467237 hasPublicationYear "2007" @default.
- W2137467237 type Work @default.
- W2137467237 sameAs 2137467237 @default.
- W2137467237 citedByCount "26" @default.
- W2137467237 countsByYear W21374672372012 @default.
- W2137467237 countsByYear W21374672372013 @default.
- W2137467237 countsByYear W21374672372014 @default.
- W2137467237 countsByYear W21374672372015 @default.
- W2137467237 countsByYear W21374672372016 @default.
- W2137467237 countsByYear W21374672372018 @default.
- W2137467237 countsByYear W21374672372019 @default.
- W2137467237 countsByYear W21374672372020 @default.
- W2137467237 countsByYear W21374672372021 @default.
- W2137467237 countsByYear W21374672372022 @default.
- W2137467237 crossrefType "journal-article" @default.
- W2137467237 hasAuthorship W2137467237A5003745554 @default.
- W2137467237 hasAuthorship W2137467237A5051687465 @default.
- W2137467237 hasAuthorship W2137467237A5081981032 @default.
- W2137467237 hasAuthorship W2137467237A5086494315 @default.
- W2137467237 hasBestOaLocation W21374672371 @default.
- W2137467237 hasConcept C121332964 @default.
- W2137467237 hasConcept C127413603 @default.
- W2137467237 hasConcept C1276947 @default.
- W2137467237 hasConcept C184665706 @default.
- W2137467237 hasConcept C44870925 @default.
- W2137467237 hasConcept C48387981 @default.
- W2137467237 hasConcept C66938386 @default.
- W2137467237 hasConcept C98444146 @default.
- W2137467237 hasConcept C99679407 @default.
- W2137467237 hasConceptScore W2137467237C121332964 @default.
- W2137467237 hasConceptScore W2137467237C127413603 @default.
- W2137467237 hasConceptScore W2137467237C1276947 @default.
- W2137467237 hasConceptScore W2137467237C184665706 @default.
- W2137467237 hasConceptScore W2137467237C44870925 @default.
- W2137467237 hasConceptScore W2137467237C48387981 @default.