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Near-IR speckle imaging of massive young stellar objects We present near-IR speckle images of 21 massive Young Stellar Objects(YSOs) associated with outflows. The aim of this study is to search forsub-arcsecond reflection nebulae associated with the outflow cavity. Wefind that 6 of the massive YSOs show a conical nebula which can beinterpreted in terms of reflected light from the dusty walls of theoutflow cavity. In all cases, the small scale structures seen in ourimages are compared with outflow indicators found in the literature. Noclear correlation is found between the presence of the reflectionnebulosity and any property such as degree of embeddedness. We also notethat 3 of the sources show close companions, one of them belonging alsoto the sample with conical nebula.Figures \ref{S140SpeckleFig}, \ref{S255SpeckleFig},\ref{Ha101Fig}-\ref{HGL490Fig} and\ref{GL2591SpeckleFig}-\ref{GL5180peckleFig} are only available inelectronic form at http://www.edpsciences.org
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| The stellar distribution in the galactic anticenter. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1967AJ.....72.1199M&db_key=AST
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Osservazione e dati astrometrici
Costellazione: | Gemelli |
Ascensione retta: | 06h07m48.63s |
Declinazione: | +22°00'09.5" |
Magnitudine apparente: | 8.521 |
Distanza: | 114.548 parsec |
Moto proprio RA: | 49.6 |
Moto proprio Dec: | -55.8 |
B-T magnitude: | 9.121 |
V-T magnitude: | 8.571 |
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