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• W3100465475 endingPage "61" @default.
• W3100465475 startingPage "61" @default.
• W3100465475 abstract "ALMA surveys of nearby star-forming regions have shown that the dust mass in the disk is correlated with the stellar mass, but with a large scatter. This scatter could indicate either different evolutionary paths of disks or different initial conditions within a single cluster. We present ALMA Cycle 3 follow-up observations for 14 Class II disks that were low S/N detections or non-detections in our Cycle 2 survey of the $sim 2$ Myr-old Chamaeleon I star-forming region. With 5 times better sensitivity, we detect millimeter dust continuum emission from six more sources and increase the detection rate to 94% (51/54) for Chamaeleon I disks around stars earlier than M3. The stellar-disk mass scaling relation reported in citet{pascucci2016} is confirmed with these updated measurements. Faint outliers in the $F_{mm}$--$M_*$ plane include three non-detections (CHXR71, CHXR30A, and T54) with dust mass upper limits of 0.2 M$_oplus$ and three very faint disks (CHXR20, ISO91, and T51) with dust masses $sim 0.5$ M$_oplus$. By investigating the SED morphology, accretion property and stellar multiplicity, we suggest for the three millimeter non-detections that tidal interaction by a close companion ($<$100 AU) and internal photoevaporation may play a role in hastening the overall disk evolution. The presence of a disk around only the secondary star in a binary system may explain the observed stellar SEDs and low disk masses for some systems." @default.
• W3100465475 created "2020-11-23" @default.
• W3100465475 creator A5021903490 @default.
• W3100465475 creator A5028513488 @default.
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• W3100465475 creator A5090482272 @default.
• W3100465475 date "2018-08-09" @default.
• W3100465475 modified "2023-10-18" @default.
• W3100465475 title "An ALMA Survey of Faint Disks in the Chamaeleon I Star-forming Region: Why Are Some Class II Disks so Faint?" @default.
• W3100465475 cites W1635732068 @default.
• W3100465475 cites W1836950185 @default.
• W3100465475 cites W1856252200 @default.
• W3100465475 cites W1856590628 @default.
• W3100465475 cites W1883299030 @default.
• W3100465475 cites W1973652382 @default.
• W3100465475 cites W1981001851 @default.
• W3100465475 cites W1982164286 @default.
• W3100465475 cites W1985404912 @default.
• W3100465475 cites W1986743369 @default.
• W3100465475 cites W1989154588 @default.
• W3100465475 cites W1989828771 @default.
• W3100465475 cites W1993037581 @default.
• W3100465475 cites W1994517704 @default.
• W3100465475 cites W1995709019 @default.
• W3100465475 cites W1998757246 @default.
• W3100465475 cites W2000562328 @default.
• W3100465475 cites W2005927107 @default.
• W3100465475 cites W2009273338 @default.
• W3100465475 cites W2012465054 @default.
• W3100465475 cites W2014960797 @default.
• W3100465475 cites W2023574719 @default.
• W3100465475 cites W2025337948 @default.
• W3100465475 cites W2026604215 @default.
• W3100465475 cites W2026780118 @default.
• W3100465475 cites W2030641521 @default.
• W3100465475 cites W2036448523 @default.
• W3100465475 cites W2041475839 @default.
• W3100465475 cites W2047309141 @default.
• W3100465475 cites W2049996606 @default.
• W3100465475 cites W2050538863 @default.
• W3100465475 cites W2053391770 @default.
• W3100465475 cites W2056887900 @default.
• W3100465475 cites W2068433364 @default.
• W3100465475 cites W2074648364 @default.
• W3100465475 cites W2077028773 @default.
• W3100465475 cites W2080259092 @default.
• W3100465475 cites W2088816706 @default.
• W3100465475 cites W2091777812 @default.
• W3100465475 cites W2105482436 @default.
• W3100465475 cites W2134663773 @default.
• W3100465475 cites W2137201296 @default.
• W3100465475 cites W2142220522 @default.
• W3100465475 cites W2145988944 @default.
• W3100465475 cites W2146591240 @default.
• W3100465475 cites W2148978321 @default.
• W3100465475 cites W2150653882 @default.
• W3100465475 cites W2154092642 @default.
• W3100465475 cites W2160161987 @default.
• W3100465475 cites W2161341103 @default.
• W3100465475 cites W2167911977 @default.
• W3100465475 cites W2170624850 @default.
• W3100465475 cites W2194952902 @default.
• W3100465475 cites W2395172868 @default.
• W3100465475 cites W2603714687 @default.
• W3100465475 cites W2604724397 @default.
• W3100465475 cites W2625453071 @default.
• W3100465475 cites W2625480451 @default.
• W3100465475 cites W2751268900 @default.
• W3100465475 cites W2751316663 @default.
• W3100465475 cites W2761954716 @default.
• W3100465475 cites W2766252874 @default.
• W3100465475 cites W2766548900 @default.
• W3100465475 cites W2949151834 @default.
• W3100465475 cites W3037126510 @default.
• W3100465475 cites W3098002080 @default.
• W3100465475 cites W3098077360 @default.
• W3100465475 cites W3098215709 @default.
• W3100465475 cites W3098259778 @default.
• W3100465475 cites W3098270532 @default.
• W3100465475 cites W3098307327 @default.
• W3100465475 cites W3098378986 @default.
• W3100465475 cites W3099176984 @default.
• W3100465475 cites W3099342797 @default.
• W3100465475 cites W3100063224 @default.
• W3100465475 cites W3100689422 @default.
• W3100465475 cites W3100855054 @default.
• W3100465475 cites W3101303225 @default.
• W3100465475 cites W3101534813 @default.
• W3100465475 cites W3101539841 @default.
• W3100465475 cites W3101656867 @default.
• W3100465475 cites W3102083771 @default.
• W3100465475 cites W3102115841 @default.
• W3100465475 cites W3102475088 @default.

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