FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1835641921> ?p ?o ?g. }

• W1835641921 abstract "In this paper we present the results of optical high-resolution imaging and spectroscopy of the complex planetary nebula (PN) NGC~3242. Our study is based on the analysis of the narrowband H$alpha$ $lambda$6563AA , [O III] $lambda$5007AA , [N II] $lambda$6584AA , and [S II] $lambda$6724{AA} images, and high- resolution spectroscopy using spectral ranges centered on the H$alpha$ $lambda$6564AA , [N II] $lambda$6583AA , and [O III] $lambda$5007AA . We detected and analysed morphological components beyond the multiple shell structure of this PN, to investigate the small-scale morphological components aligned towards its major axis (such as knots and ansae, as well as the arc-like features) and its surroundings. Thus, we investigated the morpho-kinematical properties of NGC~3242, as well as their nature and formation. Our results regarding the elliptical double-shell structure and the distance to this nebula are in concordance with previous studies. Furthermore, we have used the software SHAPE to construct a 3D model of NGC~3242, allowing us to successfully reproduce our observational data. We conclude that the prominent knots emitting in the [N II] line are fast, low-ionisation emission regions (FLIERs) related to high velocity jets and the so-called ansae-like features rather resemble bubbles. The disruptions immersed in the halo, whose emission was detected in the the [O III] high-excitation emission line, remarkably display high velocities and were formed likely in an earlier ejection event, in comparison to the innermost FLIERs and bubbles. Finally, according to our model, the kinematical ages of the structures in NGC~3242 range from 390 to 5400 yr." @default.
• W1835641921 created "2016-06-24" @default.
• W1835641921 creator A5008137476 @default.
• W1835641921 creator A5013179517 @default.
• W1835641921 creator A5018180176 @default.
• W1835641921 creator A5046184163 @default.
• W1835641921 creator A5061777170 @default.
• W1835641921 creator A5074384446 @default.
• W1835641921 date "2015-09-15" @default.
• W1835641921 modified "2023-10-03" @default.
• W1835641921 title "Morpho-kinematics of the planetary nebula NGC 3242: an analysis beyond its multiple-shell structure" @default.
• W1835641921 cites W1535662833 @default.
• W1835641921 cites W1987491699 @default.
• W1835641921 cites W1987536564 @default.
• W1835641921 cites W2000670930 @default.
• W1835641921 cites W2003666681 @default.
• W1835641921 cites W2016972318 @default.
• W1835641921 cites W2019256477 @default.
• W1835641921 cites W2028068504 @default.
• W1835641921 cites W2032069183 @default.
• W1835641921 cites W2052984037 @default.
• W1835641921 cites W2107224136 @default.
• W1835641921 cites W2113561748 @default.
• W1835641921 cites W2134841294 @default.
• W1835641921 cites W2329434860 @default.
• W1835641921 cites W2616330056 @default.
• W1835641921 cites W2950201975 @default.
• W1835641921 cites W3098580070 @default.
• W1835641921 cites W3098984831 @default.
• W1835641921 cites W3100490432 @default.
• W1835641921 cites W3102878988 @default.
• W1835641921 cites W3103117372 @default.
• W1835641921 cites W3104331331 @default.
• W1835641921 cites W85711916 @default.
• W1835641921 cites W86525955 @default.
• W1835641921 doi "https://doi.org/10.1093/mnras/stv1922" @default.
• W1835641921 hasPublicationYear "2015" @default.
• W1835641921 type Work @default.
• W1835641921 sameAs 1835641921 @default.
• W1835641921 citedByCount "8" @default.
• W1835641921 countsByYear W18356419212015 @default.
• W1835641921 countsByYear W18356419212016 @default.
• W1835641921 countsByYear W18356419212018 @default.
• W1835641921 countsByYear W18356419212019 @default.
• W1835641921 countsByYear W18356419212020 @default.
• W1835641921 crossrefType "journal-article" @default.
• W1835641921 hasAuthorship W1835641921A5008137476 @default.
• W1835641921 hasAuthorship W1835641921A5013179517 @default.
• W1835641921 hasAuthorship W1835641921A5018180176 @default.
• W1835641921 hasAuthorship W1835641921A5046184163 @default.
• W1835641921 hasAuthorship W1835641921A5061777170 @default.
• W1835641921 hasAuthorship W1835641921A5074384446 @default.
• W1835641921 hasBestOaLocation W18356419211 @default.
• W1835641921 hasConcept C120665830 @default.
• W1835641921 hasConcept C121332964 @default.
• W1835641921 hasConcept C1276947 @default.
• W1835641921 hasConcept C150846664 @default.
• W1835641921 hasConcept C173220165 @default.
• W1835641921 hasConcept C184665706 @default.
• W1835641921 hasConcept C198352243 @default.
• W1835641921 hasConcept C2524010 @default.
• W1835641921 hasConcept C26141928 @default.
• W1835641921 hasConcept C2778113609 @default.
• W1835641921 hasConcept C2779496878 @default.
• W1835641921 hasConcept C32891209 @default.
• W1835641921 hasConcept C33923547 @default.
• W1835641921 hasConcept C41074950 @default.
• W1835641921 hasConcept C44870925 @default.
• W1835641921 hasConcept C4839761 @default.
• W1835641921 hasConcept C95373548 @default.
• W1835641921 hasConcept C96141758 @default.
• W1835641921 hasConcept C98444146 @default.
• W1835641921 hasConceptScore W1835641921C120665830 @default.
• W1835641921 hasConceptScore W1835641921C121332964 @default.
• W1835641921 hasConceptScore W1835641921C1276947 @default.
• W1835641921 hasConceptScore W1835641921C150846664 @default.
• W1835641921 hasConceptScore W1835641921C173220165 @default.
• W1835641921 hasConceptScore W1835641921C184665706 @default.
• W1835641921 hasConceptScore W1835641921C198352243 @default.
• W1835641921 hasConceptScore W1835641921C2524010 @default.
• W1835641921 hasConceptScore W1835641921C26141928 @default.
• W1835641921 hasConceptScore W1835641921C2778113609 @default.
• W1835641921 hasConceptScore W1835641921C2779496878 @default.
• W1835641921 hasConceptScore W1835641921C32891209 @default.
• W1835641921 hasConceptScore W1835641921C33923547 @default.
• W1835641921 hasConceptScore W1835641921C41074950 @default.
• W1835641921 hasConceptScore W1835641921C44870925 @default.
• W1835641921 hasConceptScore W1835641921C4839761 @default.
• W1835641921 hasConceptScore W1835641921C95373548 @default.
• W1835641921 hasConceptScore W1835641921C96141758 @default.
• W1835641921 hasConceptScore W1835641921C98444146 @default.
• W1835641921 hasLocation W18356419211 @default.
• W1835641921 hasLocation W18356419212 @default.
• W1835641921 hasOpenAccess W1835641921 @default.
• W1835641921 hasPrimaryLocation W18356419211 @default.
• W1835641921 hasRelatedWork W1506565227 @default.
• W1835641921 hasRelatedWork W1971768081 @default.
• W1835641921 hasRelatedWork W1981322587 @default.
• W1835641921 hasRelatedWork W1987491699 @default.
• W1835641921 hasRelatedWork W2007454166 @default.

• next