FAUST: IX. Multiband, multiscale dust study of L1527 IRS. Evidence for variations in dust properties within the envelope of a class 0/I young stellar object

Author(s):
Cacciapuoti, L.; Macias, E.; Maury, A.J.; Chandler, C.J.; Sakai, N.; Tychoniec, Ł.; Viti, S. (0000-0001-8504-8844); Natta, A.; De Simone, M.; Miotello, A.; Codella, C.; Ceccarelli, C.; Podio, L.; Fedele, D.; Johnstone, D.; Shirley, Y.; Liu, B.J.; Bianchi, E.; Zhang, Z.E.; Pineda, J.; Loinard, L.; Ménard, F.; Lebreuilly, U.; Klessen, R.S.; Hennebelle, P.; Molinari, S.; Testi, L.; Yamamoto, S.
Published
2023
Publication type
Article / Letter to editor
Planets and satellites: formationProtoplanetary disksTechniques: interferometricDustExtinctionSubmillimeter: planetary systemsSubmillimeter: ISMAstrophysics - Solar and Stellar AstrophysicsAstrophysics - Earth and Planetary AstrophysicsAstrophysics - Astrophysics of Galaxies
Date issued
2023
Language
English
Is part of
Astronomy and Astrophysics (2023), A4
hdl
1887/3717995
doi
10.1051/0004-6361/202346204
URL
https://ui.adsabs.harvard.edu/abs/2023A&A...676A...4C