Matches in SemOpenAlex for { <https://semopenalex.org/work/W2023240185> ?p ?o ?g. }
- W2023240185 endingPage "2426" @default.
- W2023240185 startingPage "2411" @default.
- W2023240185 abstract "We present adaptive optics-assisted J- and K-band integral field spectroscopy of the inner 300 x 300 pc of the Seyfert 2 galaxy NGC1068. The data were obtained with the Gemini NIFS integral field unit spectrometer, which provided us with high-spatial and -spectral resolution sampling. The wavelength range covered by the observations allowed us to study the [CaVIII], [SiVI], [SiVII], [AlIX] and [SIX] coronal-line (CL) emission, covering ionization potentials up to 328 eV. The observations reveal very rich and complex structures, both in terms of velocity fields and emission-line ratios. The CL emission is elongated along the NE-SW direction, with the stronger emission preferentially localized to the NE of the nucleus. CLs are emitted by gas covering a wide range of velocities, with maximum blueshifts/redshifts of ~ -1600/1000 km/s. There is a trend for the gas located on the NE side of the nucleus to be blueshifted while the gas located towards the SW is redshifted. The morphology and the kinematics of the near-infrared CLs are in very good agreement with the ones displayed by low-ionization lines and optical CLs, suggesting a common origin. The line flux distributions, velocity maps, ionization structure (traced by the [SiVII]/[SiVI] emission-line ratio) and low ionization emission-line ratios (i.e., [FeII]/Pabeta and [FeII]/[PII]) suggest that the radio jet plays an important role in the structure of the coronal line region of this object, and possibly in its kinematics." @default.
- W2023240185 created "2016-06-24" @default.
- W2023240185 creator A5022376918 @default.
- W2023240185 creator A5044060390 @default.
- W2023240185 creator A5061222158 @default.
- W2023240185 creator A5083220430 @default.
- W2023240185 date "2013-02-14" @default.
- W2023240185 modified "2023-09-26" @default.
- W2023240185 title "Resolving the coronal line region of NGC 1068 with near-infrared integral field spectroscopy★" @default.
- W2023240185 cites W1613611297 @default.
- W2023240185 cites W1645651125 @default.
- W2023240185 cites W1882938068 @default.
- W2023240185 cites W1974437338 @default.
- W2023240185 cites W1975244579 @default.
- W2023240185 cites W1982223538 @default.
- W2023240185 cites W1985321813 @default.
- W2023240185 cites W1985726073 @default.
- W2023240185 cites W1986161569 @default.
- W2023240185 cites W1999818838 @default.
- W2023240185 cites W2009794248 @default.
- W2023240185 cites W2017862978 @default.
- W2023240185 cites W2019676304 @default.
- W2023240185 cites W2021128232 @default.
- W2023240185 cites W2024549158 @default.
- W2023240185 cites W2028072322 @default.
- W2023240185 cites W2030574107 @default.
- W2023240185 cites W2040313811 @default.
- W2023240185 cites W2041721739 @default.
- W2023240185 cites W2042737625 @default.
- W2023240185 cites W2045974263 @default.
- W2023240185 cites W2049592378 @default.
- W2023240185 cites W2050463902 @default.
- W2023240185 cites W2052009095 @default.
- W2023240185 cites W2053483836 @default.
- W2023240185 cites W2058697899 @default.
- W2023240185 cites W2058865883 @default.
- W2023240185 cites W2063744623 @default.
- W2023240185 cites W2071508523 @default.
- W2023240185 cites W2071702124 @default.
- W2023240185 cites W2072905490 @default.
- W2023240185 cites W2084260861 @default.
- W2023240185 cites W2093015804 @default.
- W2023240185 cites W2094212119 @default.
- W2023240185 cites W2105658132 @default.
- W2023240185 cites W2111979057 @default.
- W2023240185 cites W2130478079 @default.
- W2023240185 cites W2152697521 @default.
- W2023240185 cites W2158724634 @default.
- W2023240185 cites W2158750970 @default.
- W2023240185 cites W2170897440 @default.
- W2023240185 cites W2315610640 @default.
- W2023240185 cites W2335240673 @default.
- W2023240185 cites W2951323278 @default.
- W2023240185 cites W3099497158 @default.
- W2023240185 cites W3099510388 @default.
- W2023240185 cites W3100732492 @default.
- W2023240185 cites W3101596395 @default.
- W2023240185 cites W3101943668 @default.
- W2023240185 cites W3102822082 @default.
- W2023240185 cites W3103611272 @default.
- W2023240185 cites W3105293888 @default.
- W2023240185 cites W3105660388 @default.
- W2023240185 cites W3106298542 @default.
- W2023240185 cites W3106329246 @default.
- W2023240185 cites W4302778843 @default.
- W2023240185 doi "https://doi.org/10.1093/mnras/stt064" @default.
- W2023240185 hasPublicationYear "2013" @default.
- W2023240185 type Work @default.
- W2023240185 sameAs 2023240185 @default.
- W2023240185 citedByCount "28" @default.
- W2023240185 countsByYear W20232401852013 @default.
- W2023240185 countsByYear W20232401852014 @default.
- W2023240185 countsByYear W20232401852015 @default.
- W2023240185 countsByYear W20232401852016 @default.
- W2023240185 countsByYear W20232401852017 @default.
- W2023240185 countsByYear W20232401852018 @default.
- W2023240185 countsByYear W20232401852021 @default.
- W2023240185 countsByYear W20232401852022 @default.
- W2023240185 crossrefType "journal-article" @default.
- W2023240185 hasAuthorship W2023240185A5022376918 @default.
- W2023240185 hasAuthorship W2023240185A5044060390 @default.
- W2023240185 hasAuthorship W2023240185A5061222158 @default.
- W2023240185 hasAuthorship W2023240185A5083220430 @default.
- W2023240185 hasBestOaLocation W20232401851 @default.
- W2023240185 hasConcept C121332964 @default.
- W2023240185 hasConcept C124967146 @default.
- W2023240185 hasConcept C1276947 @default.
- W2023240185 hasConcept C145148216 @default.
- W2023240185 hasConcept C158355884 @default.
- W2023240185 hasConcept C198291218 @default.
- W2023240185 hasConcept C198352243 @default.
- W2023240185 hasConcept C2524010 @default.
- W2023240185 hasConcept C32891209 @default.
- W2023240185 hasConcept C33024259 @default.
- W2023240185 hasConcept C33923547 @default.
- W2023240185 hasConcept C43481613 @default.
- W2023240185 hasConcept C44870925 @default.
- W2023240185 hasConcept C4839761 @default.