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• W3105227515 abstract "We present continuum and molecular line observations at 230 GHz and 345 GHz from the Sub-millimeter Array (SMA) toward three protostars in the Perseus L1448N region. The data are from the large project Mass Assembly of Stellar Systems and their Evolution with the SMA (MASSES). Three dust continuum sources, Source B, Source NW, and Source A, are detected at both frequencies. These sources have corresponding emission peaks in C18O (J=2-1), 13CO (J=2-1), and HCO+ (J=4-3), and have offsets with N2D+ (J=3-2) peaks. High angular resolution data from a complimentary continuum survey with the Karl G. Jansky Very Large Array show that Source B is associated with three 8 mm continuum objects, Source NW with two, and Source A remains single. These results suggest that multiplicity in L1448N exists at different spatial scales from a few thousand AU to < 100 AU. Velocity gradients in each source obtained from two-dimensional fits to the SMA C18O emission are found to be perpendicular to within 20 degrees of the outflow directions as revealed by 12CO (J=2-1). We have observed that Sources B and NW with multiplicity have higher densities than Source A without multiplicity. This suggests that thermal Jeans fragmentation can be relevant in the fragmentation process. However, we have not observed a difference in the ratio between rotational and gravitational energy between sources with and without multiplicity. We also have not observed a trend between non-thermal velocity dispersions and the level of fragmentation. Our study has provided the first direct and comprehensive comparison between multiplicity and core properties in low-mass protostars, although based on small number statistics." @default.
• W3105227515 created "2020-11-23" @default.
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• W3105227515 date "2015-11-23" @default.
• W3105227515 modified "2023-10-17" @default.
• W3105227515 title "MASS ASSEMBLY OF STELLAR SYSTEMS AND THEIR EVOLUTION WITH THE SMA (MASSES). MULTIPLICITY AND THE PHYSICAL ENVIRONMENT IN L1448N" @default.
• W3105227515 cites W1621338982 @default.
• W3105227515 cites W1929501738 @default.
• W3105227515 cites W1974671582 @default.
• W3105227515 cites W1976071602 @default.
• W3105227515 cites W1984518272 @default.
• W3105227515 cites W1986202073 @default.
• W3105227515 cites W1987546210 @default.
• W3105227515 cites W2008783600 @default.
• W3105227515 cites W2011317418 @default.
• W3105227515 cites W2014137776 @default.
• W3105227515 cites W2018609579 @default.
• W3105227515 cites W2020817247 @default.
• W3105227515 cites W2024173203 @default.
• W3105227515 cites W2030361765 @default.
• W3105227515 cites W2030792825 @default.
• W3105227515 cites W2031301935 @default.
• W3105227515 cites W2032439527 @default.
• W3105227515 cites W2034255580 @default.
• W3105227515 cites W2034332576 @default.
• W3105227515 cites W2036179433 @default.
• W3105227515 cites W2036806513 @default.
• W3105227515 cites W2046009229 @default.
• W3105227515 cites W2046452618 @default.
• W3105227515 cites W2046957257 @default.
• W3105227515 cites W2048498057 @default.
• W3105227515 cites W2048921969 @default.
• W3105227515 cites W2049098853 @default.
• W3105227515 cites W2051431923 @default.
• W3105227515 cites W2056671836 @default.
• W3105227515 cites W2061605769 @default.
• W3105227515 cites W2062854143 @default.
• W3105227515 cites W2072019403 @default.
• W3105227515 cites W2079349148 @default.
• W3105227515 cites W2082971238 @default.
• W3105227515 cites W2086373253 @default.
• W3105227515 cites W2089176910 @default.
• W3105227515 cites W2089629734 @default.
• W3105227515 cites W2092659903 @default.
• W3105227515 cites W2093342937 @default.
• W3105227515 cites W2096191227 @default.
• W3105227515 cites W2097578502 @default.
• W3105227515 cites W2112354520 @default.
• W3105227515 cites W2113912459 @default.
• W3105227515 cites W2116276870 @default.
• W3105227515 cites W2128599863 @default.
• W3105227515 cites W2134478144 @default.
• W3105227515 cites W2135671800 @default.
• W3105227515 cites W2140220905 @default.
• W3105227515 cites W2146896318 @default.
• W3105227515 cites W2152276979 @default.
• W3105227515 cites W2162460629 @default.
• W3105227515 cites W2163097250 @default.
• W3105227515 cites W2166857071 @default.
• W3105227515 cites W2168179538 @default.
• W3105227515 cites W2170204004 @default.
• W3105227515 cites W2736152241 @default.
• W3105227515 cites W2964257340 @default.
• W3105227515 cites W3037126510 @default.
• W3105227515 cites W3098135919 @default.
• W3105227515 cites W3098592720 @default.
• W3105227515 cites W3099015392 @default.
• W3105227515 cites W3099135685 @default.
• W3105227515 cites W3100060537 @default.
• W3105227515 cites W3100345724 @default.
• W3105227515 cites W3101145158 @default.
• W3105227515 cites W3102263934 @default.
• W3105227515 cites W3102280935 @default.
• W3105227515 cites W3102386126 @default.
• W3105227515 cites W3103791584 @default.
• W3105227515 cites W3104001783 @default.
• W3105227515 cites W3104232687 @default.
• W3105227515 cites W3104505809 @default.

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