eprintid: 10192158 rev_number: 7 eprint_status: archive userid: 699 dir: disk0/10/19/21/58 datestamp: 2024-05-13 14:27:22 lastmod: 2024-05-13 14:27:22 status_changed: 2024-05-13 14:27:22 type: article metadata_visibility: show sword_depositor: 699 creators_name: Garufi, A creators_name: Ginski, C creators_name: van Holstein, RG creators_name: Benisty, M creators_name: Manara, CF creators_name: Pérez, S creators_name: Pinilla, P creators_name: Ribas, Á creators_name: Weber, P creators_name: Williams, J creators_name: Cieza, L creators_name: Dominik, C creators_name: Facchini, S creators_name: Huang, J creators_name: Zurlo, A creators_name: Bae, J creators_name: Hagelberg, J creators_name: Henning, Th creators_name: Hogerheijde, MR creators_name: Janson, M creators_name: Ménard, F creators_name: Messina, S creators_name: Meyer, MR creators_name: Pinte, C creators_name: Quanz, SP creators_name: Rigliaco, E creators_name: Roccatagliata, V creators_name: Schmid, HM creators_name: Szulágyi, J creators_name: van Boekel, R creators_name: Wahhaj, Z creators_name: Antichi, J creators_name: Baruffolo, A creators_name: Moulin, T title: The SPHERE view of the Taurus star-forming region ispublished: pub divisions: UCL divisions: B04 divisions: C06 divisions: F63 keywords: Techniques: polarimetric, protoplanetary disks, stars: pre-main sequence note: Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. abstract: The sample of planet-forming disks observed by high-contrast imaging campaigns over the last decade is mature enough to enable the demographical analysis of individual star-forming regions. We present the full census of Taurus sources with VLT/SPHERE polarimetric images available. The whole sample sums up to 43 targets (of which 31 have not been previously published) corresponding to one-fifth of the Class II population in Taurus and about half of such objects that are observable. A large fraction of the sample is apparently made up of isolated faint disks (equally divided between small and large self-shadowed disks). Ambient signal is visible in about one-third of the sample. This probes the interaction with the environment and with companions or the outflow activity of the system. The central portion of the Taurus region almost exclusively hosts faint disks, while the periphery also hosts bright disks interacting with their surroundings. The few bright disks are found around apparently older stars. The overall picture is that the Taurus region is in an early evolutionary stage of planet formation. Yet, some objects are discussed individually, as in an intermediate or exceptional stage of the disk evolution. This census provides a first benchmark for the comparison of the disk populations in different star forming regions. date: 2024-05 date_type: published publisher: EDP Sciences official_url: https://doi.org/10.1051/0004-6361/202347586 oa_status: green full_text_type: pub language: eng primo: open primo_central: open_green verified: verified_manual elements_id: 2274324 doi: 10.1051/0004-6361/202347586 lyricists_name: Pinilla, Paola lyricists_id: PPINI88 actors_name: Flynn, Bernadette actors_id: BFFLY94 actors_role: owner full_text_status: public publication: Astronomy & Astrophysics volume: 685 article_number: A53 issn: 0004-6361 citation: Garufi, A; Ginski, C; van Holstein, RG; Benisty, M; Manara, CF; Pérez, S; Pinilla, P; ... Moulin, T; + view all <#> Garufi, A; Ginski, C; van Holstein, RG; Benisty, M; Manara, CF; Pérez, S; Pinilla, P; Ribas, Á; Weber, P; Williams, J; Cieza, L; Dominik, C; Facchini, S; Huang, J; Zurlo, A; Bae, J; Hagelberg, J; Henning, Th; Hogerheijde, MR; Janson, M; Ménard, F; Messina, S; Meyer, MR; Pinte, C; Quanz, SP; Rigliaco, E; Roccatagliata, V; Schmid, HM; Szulágyi, J; van Boekel, R; Wahhaj, Z; Antichi, J; Baruffolo, A; Moulin, T; - view fewer <#> (2024) The SPHERE view of the Taurus star-forming region. Astronomy & Astrophysics , 685 , Article A53. 10.1051/0004-6361/202347586 <https://doi.org/10.1051/0004-6361%2F202347586>. Green open access document_url: https://discovery.ucl.ac.uk/id/eprint/10192158/1/aa47586-23.pdf