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- W2891687906 abstract "The Herschel Gould Belt Survey key project mapped the bulk of nearby star-forming molecular clouds in five far-infrared bands with the aim of compiling complete census of prestellar cores and young, embedded protostars. In this paper, we present the catalogue of the dense cores and YSOs/protostars extracted from the Herschel maps of the Lupus I, III, and IV molecular clouds. The physical properties of the detected objects were derived by fitting their spectral energy distributions. A total of 532 dense cores, out of which 103 are presumably prestellar in nature, and 38 YSOs/protostars have been detected in the three clouds. Almost all the prestellar cores are associated with filaments against only about one third of the unbound cores and YSOs/protostars. Prestellar core candidates are found even in filaments that are on average thermally sub-critical and over a background column density lower than that measured in other star forming regions so far. The core mass function of the prestellar cores peaks between 0.2 and 0.3 solar masses and it is compatible with the log-normal shape found in other regions. Herschel data reveal several, previously undetected, protostars and new candidates of Class 0 and Class II with transitional disks. We estimate the evolutionary status of the YSOs/protostars using two independent indicators: the $alpha$ index and the fitting of the spectral energy distribution from near- to far-infrared wavelengths. For 70% of the objects, the evolutionary stages derived with the two methods are in agreement. Lupus is confirmed to be a very low-mass star-forming region, both in terms of the prestellar condensations and of the diffuse medium. Noticeably, in the Lupus clouds we have found star formation activity associated with interstellar medium at low column density, usually quiescent in other (more massive) star forming regions." @default.
- W2891687906 created "2018-09-27" @default.
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- W2891687906 date "2018-10-31" @default.
- W2891687906 modified "2023-10-02" @default.
- W2891687906 title "A catalogue of dense cores and young stellar objects in the Lupus complex based on <i>Herschel</i> Gould Belt Survey observations" @default.
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- W2891687906 cites W1644389388 @default.
- W2891687906 cites W1668907131 @default.
- W2891687906 cites W1966842402 @default.
- W2891687906 cites W1970066316 @default.
- W2891687906 cites W1983264191 @default.
- W2891687906 cites W1985647485 @default.
- W2891687906 cites W2000672249 @default.
- W2891687906 cites W2009132417 @default.
- W2891687906 cites W2011090989 @default.
- W2891687906 cites W2016573758 @default.
- W2891687906 cites W2019579421 @default.
- W2891687906 cites W2024173203 @default.
- W2891687906 cites W2028181754 @default.
- W2891687906 cites W2032986063 @default.
- W2891687906 cites W2074299830 @default.
- W2891687906 cites W2082029417 @default.
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- W2891687906 cites W2093034564 @default.
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- W2891687906 cites W2132251019 @default.
- W2891687906 cites W2133815176 @default.
- W2891687906 cites W2133991519 @default.
- W2891687906 cites W2135536375 @default.
- W2891687906 cites W2136310247 @default.
- W2891687906 cites W2148165343 @default.
- W2891687906 cites W2148681289 @default.
- W2891687906 cites W2151139906 @default.
- W2891687906 cites W2154298686 @default.
- W2891687906 cites W2171603061 @default.
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- W2891687906 cites W2437780333 @default.
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- W2891687906 cites W2760851005 @default.
- W2891687906 cites W3098252123 @default.
- W2891687906 cites W3098271229 @default.
- W2891687906 cites W3098653307 @default.
- W2891687906 cites W3099758489 @default.
- W2891687906 cites W3100106758 @default.
- W2891687906 cites W3100801896 @default.
- W2891687906 cites W3101077767 @default.
- W2891687906 cites W3101550428 @default.
- W2891687906 cites W3102398079 @default.
- W2891687906 cites W3102521950 @default.
- W2891687906 cites W3103730889 @default.
- W2891687906 cites W3104423841 @default.
- W2891687906 cites W3104571529 @default.
- W2891687906 cites W3105119744 @default.
- W2891687906 cites W3106047177 @default.
- W2891687906 cites W3106485099 @default.
- W2891687906 cites W3121634870 @default.
- W2891687906 cites W3125901853 @default.
- W2891687906 cites W4289710459 @default.
- W2891687906 cites W4289815540 @default.
- W2891687906 cites W4292403301 @default.
- W2891687906 cites W4293003757 @default.
- W2891687906 cites W4297832571 @default.
- W2891687906 cites W4300487395 @default.
- W2891687906 cites W4301509784 @default.
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- W2891687906 doi "https://doi.org/10.1051/0004-6361/201833364" @default.
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