The disk substructures at high angular resolution project (DSHARP). I. Motivation, sample, calibration, and overview SM Andrews, J Huang, LM Pérez, A Isella, CP Dullemond, NT Kurtovic, ... The Astrophysical Journal Letters 869 (2), L41, 2018 | 805 | 2018 |
Ringed substructure and a gap at 1 au in the nearest protoplanetary disk SM Andrews, DJ Wilner, Z Zhu, T Birnstiel, JM Carpenter, LM Pérez, ... The Astrophysical Journal Letters 820 (2), L40, 2016 | 438 | 2016 |
Dust filtration by planet-induced gap edges: implications for transitional disks Z Zhu, RP Nelson, R Dong, C Espaillat, L Hartmann The Astrophysical Journal 755 (1), 6, 2012 | 427 | 2012 |
The disk substructures at high angular resolution project (DSHARP). VI. Dust trapping in thin-ringed protoplanetary disks CP Dullemond, T Birnstiel, J Huang, NT Kurtovic, SM Andrews, ... The Astrophysical Journal Letters 869 (2), L46, 2018 | 401 | 2018 |
Transitional and pre-transitional disks: gap opening by multiple planets? Z Zhu, RP Nelson, L Hartmann, C Espaillat, N Calvet The Astrophysical Journal 729 (1), 47, 2011 | 357 | 2011 |
Episodic accretion in young stars M Audard, P Abrahám, MM Dunham, JD Green, N Grosso, K Hamaguchi, ... Protostars and planets VI 387 (1401.3368), 2014 | 345 | 2014 |
The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA maps of protoplanetary disks in terms of a dust model T Birnstiel, CP Dullemond, Z Zhu, SM Andrews, XN Bai, DJ Wilner, ... The Astrophysical Journal Letters 869 (2), L45, 2018 | 330 | 2018 |
The disk substructures at high angular resolution project (DSHARP). II. Characteristics of annular substructures J Huang, SM Andrews, CP Dullemond, A Isella, LM Pérez, VV Guzmán, ... The Astrophysical Journal Letters 869 (2), L42, 2018 | 308 | 2018 |
An observational perspective of transitional disks C Espaillat, J Muzerolle, J Najita, S Andrews, Z Zhu, N Calvet, S Kraus, ... arXiv preprint arXiv:1402.7103, 2014 | 308 | 2014 |
Observational signatures of planets in protoplanetary disks. I. Gaps opened by single and multiple young planets in disks R Dong, Z Zhu, B Whitney The Astrophysical Journal 809 (1), 93, 2015 | 290 | 2015 |
The disk substructures at high angular resolution project (DSHARP). VII. The planet–disk interactions interpretation S Zhang, Z Zhu, J Huang, VV Guzmán, SM Andrews, T Birnstiel, ... The Astrophysical Journal Letters 869 (2), L47, 2018 | 288 | 2018 |
Nonsteady accretion in protostars Z Zhu, L Hartmann, C Gammie The Astrophysical Journal 694 (2), 1045, 2009 | 263 | 2009 |
Exoplanet orbital eccentricities derived from LAMOST–Kepler analysis JW Xie, S Dong, Z Zhu, D Huber, Z Zheng, P De Cat, J Fu, HG Liu, A Luo, ... Proceedings of the National Academy of Sciences 113 (41), 11431-11435, 2016 | 262 | 2016 |
Challenges in forming planets by gravitational instability: disk irradiation and clump migration, accretion, and tidal destruction Z Zhu, L Hartmann, RP Nelson, CF Gammie The Astrophysical Journal 746 (1), 110, 2012 | 242 | 2012 |
Imaging the water snow-line during a protostellar outburst LA Cieza, S Casassus, J Tobin, SP Bos, JP Williams, S Perez, Z Zhu, ... Nature 535 (7611), 258-261, 2016 | 241 | 2016 |
The structure of spiral shocks excited by planetary-mass companions Z Zhu, R Dong, JM Stone, RR Rafikov The Astrophysical Journal 813 (2), 88, 2015 | 206 | 2015 |
The eccentric cavity, triple rings, two-armed spirals, and double clumps of the MWC 758 disk R Dong, S Liu, J Eisner, S Andrews, J Fung, Z Zhu, E Chiang, ... The Astrophysical Journal 860 (2), 124, 2018 | 199 | 2018 |
The Disk Substructures at High Angular Resolution Project (DSHARP). IX. A high-definition study of the HD 163296 planet-forming disk A Isella, J Huang, SM Andrews, CP Dullemond, T Birnstiel, S Zhang, ... The Astrophysical journal letters 869 (2), L49, 2018 | 198 | 2018 |
CO and dust properties in the TW Hya disk from high-resolution ALMA observations J Huang, SM Andrews, LI Cleeves, KI Öberg, DJ Wilner, X Bai, T Birnstiel, ... The Astrophysical Journal 852 (2), 122, 2018 | 195 | 2018 |
FAST RISE OF “NEPTUNE-SIZE” PLANETS (4–8 R⊕) FROM P∼ 10 TO∼ 250 DAYS—STATISTICS OF KEPLER PLANET CANDIDATES UP TO∼ 0.75 AU S Dong, Z Zhu The Astrophysical Journal 778 (1), 53, 2013 | 194 | 2013 |