Matches in SemOpenAlex for { <https://semopenalex.org/work/W1771646347> ?p ?o ?g. }
- W1771646347 endingPage "276" @default.
- W1771646347 startingPage "264" @default.
- W1771646347 abstract "We present visible and near-infrared photometry and spectroscopy of LS-RCrA 1, a faint, very late-type object (M 6.5-M 7) seen in the direction of the R Coronae Australis star forming complex. While its emission spectrum shows prominent features of accretion and mass loss typical of young stellar objects, its underlying continuum and photometric properties are puzzling when trying to derive a mass and age based on pre-main sequence evolutionary tracks: the object appears to be far too faint for a young member of the R Coronae Australis complex of its spectral type. We speculate that this may be due to either its evolution along pre-main sequence tracks being substantially altered by the intense accretion, or to a combination of partial blocking and scattering of the light of the object by a nearly edge-on circumstellar disk. The rich emission line spectrum superimposed on the stellar continuum is well explained by an intense accretion process: the Hα, CaII infrared triplet, and HeI 6678 lines show equivalent widths typical of very active classical T Tauri stars. The near-infrared observations show anomalously weak spectral features and no significant excess emission in the K band, which we tentatively interpret as indicating line filling due to emission in a magnetic accretion funnel flow. At the same time, numerous, strong forbidden optical lines ([OI], [NII] and [SII]) and H2 emission at 2.12 μm suggest that the object is simultaneously undergoing mass loss, providing another example that shows that mass loss and accretion are closely related processes. Such an intense accretion and mass loss activity is observed for the first time in a young stellar object in the transition region between low mass stars and brown dwarfs, and provides a valuable observational test on the effects of accretion on the evolution of objects with such low masses." @default.
- W1771646347 created "2016-06-24" @default.
- W1771646347 creator A5010509711 @default.
- W1771646347 creator A5068575324 @default.
- W1771646347 date "2001-12-01" @default.
- W1771646347 modified "2023-10-16" @default.
- W1771646347 title "Intense accretion and mass loss of a very low mass young stellar object" @default.
- W1771646347 cites W1502203903 @default.
- W1771646347 cites W1967340141 @default.
- W1771646347 cites W1970076709 @default.
- W1771646347 cites W1972537197 @default.
- W1771646347 cites W1975197132 @default.
- W1771646347 cites W1980976824 @default.
- W1771646347 cites W1983605281 @default.
- W1771646347 cites W1983968691 @default.
- W1771646347 cites W1985663566 @default.
- W1771646347 cites W1991502431 @default.
- W1771646347 cites W1994277384 @default.
- W1771646347 cites W2001892464 @default.
- W1771646347 cites W2006727841 @default.
- W1771646347 cites W2009029252 @default.
- W1771646347 cites W2020013679 @default.
- W1771646347 cites W2024977654 @default.
- W1771646347 cites W2026795906 @default.
- W1771646347 cites W2027542103 @default.
- W1771646347 cites W2029196460 @default.
- W1771646347 cites W2036767850 @default.
- W1771646347 cites W2042753720 @default.
- W1771646347 cites W2045793805 @default.
- W1771646347 cites W2046793067 @default.
- W1771646347 cites W2047475046 @default.
- W1771646347 cites W2049896064 @default.
- W1771646347 cites W2050340053 @default.
- W1771646347 cites W2054697790 @default.
- W1771646347 cites W2061914283 @default.
- W1771646347 cites W2064597279 @default.
- W1771646347 cites W2066533573 @default.
- W1771646347 cites W2075076813 @default.
- W1771646347 cites W2075519868 @default.
- W1771646347 cites W2078834481 @default.
- W1771646347 cites W2082612383 @default.
- W1771646347 cites W2083293100 @default.
- W1771646347 cites W2085443725 @default.
- W1771646347 cites W2086375588 @default.
- W1771646347 cites W2088202101 @default.
- W1771646347 cites W2091756692 @default.
- W1771646347 cites W2092380306 @default.
- W1771646347 cites W2095162860 @default.
- W1771646347 cites W2126142867 @default.
- W1771646347 cites W2144310152 @default.
- W1771646347 cites W2161691817 @default.
- W1771646347 cites W2173670823 @default.
- W1771646347 cites W2320120954 @default.
- W1771646347 cites W3098460303 @default.
- W1771646347 cites W3101286584 @default.
- W1771646347 cites W3106506285 @default.
- W1771646347 doi "https://doi.org/10.1051/0004-6361:20011443" @default.
- W1771646347 hasPublicationYear "2001" @default.
- W1771646347 type Work @default.
- W1771646347 sameAs 1771646347 @default.
- W1771646347 citedByCount "93" @default.
- W1771646347 countsByYear W17716463472012 @default.
- W1771646347 countsByYear W17716463472013 @default.
- W1771646347 countsByYear W17716463472014 @default.
- W1771646347 countsByYear W17716463472017 @default.
- W1771646347 countsByYear W17716463472018 @default.
- W1771646347 countsByYear W17716463472019 @default.
- W1771646347 countsByYear W17716463472020 @default.
- W1771646347 countsByYear W17716463472022 @default.
- W1771646347 crossrefType "journal-article" @default.
- W1771646347 hasAuthorship W1771646347A5010509711 @default.
- W1771646347 hasAuthorship W1771646347A5068575324 @default.
- W1771646347 hasBestOaLocation W17716463471 @default.
- W1771646347 hasConcept C120665830 @default.
- W1771646347 hasConcept C121332964 @default.
- W1771646347 hasConcept C125857072 @default.
- W1771646347 hasConcept C1276947 @default.
- W1771646347 hasConcept C150846664 @default.
- W1771646347 hasConcept C158355884 @default.
- W1771646347 hasConcept C163531172 @default.
- W1771646347 hasConcept C168589115 @default.
- W1771646347 hasConcept C178075534 @default.
- W1771646347 hasConcept C23254167 @default.
- W1771646347 hasConcept C2776401274 @default.
- W1771646347 hasConcept C2779760567 @default.
- W1771646347 hasConcept C44870925 @default.
- W1771646347 hasConcept C4839761 @default.
- W1771646347 hasConcept C60056205 @default.
- W1771646347 hasConcept C68271606 @default.
- W1771646347 hasConcept C96141758 @default.
- W1771646347 hasConceptScore W1771646347C120665830 @default.
- W1771646347 hasConceptScore W1771646347C121332964 @default.
- W1771646347 hasConceptScore W1771646347C125857072 @default.
- W1771646347 hasConceptScore W1771646347C1276947 @default.
- W1771646347 hasConceptScore W1771646347C150846664 @default.
- W1771646347 hasConceptScore W1771646347C158355884 @default.
- W1771646347 hasConceptScore W1771646347C163531172 @default.
- W1771646347 hasConceptScore W1771646347C168589115 @default.