Bajaj, N. S., Pascucci, I., Cabrit, S., Edwards, S., Cugno, G., Sellek, A. D., Najita, J. R., Zhang, K., Alexander, R., Herczeg, G. J., Gorti, U., Clark, S. C., Beck, T. L., 2026. "JWST/MIRI Reveals the Evolution from Molecular to Atomic Disk Winds", The Astronomical Journal, 172, 161.

Bajaj N. S., Pascucci I, Beck T, Edwards S, Cabrit S, Najita J, Schwarz K, Semenov D, Salyk C, Gorti U, Brittain S, Krijt S, Ruaud M, Muzerolle Page J, 2025. "Class I/II Jets with JWST: Mass-loss Rates, Asymmetries, and Binary-induced Wigglings", The Astronomical Journal, 169, 6.

Xie C, Pascucci I, Deng D, Bajaj N, Alexander R, Sellek A, Kóspál Á, Ballabio G, Gorti U, 2024. "JWST Captures a Sudden Stellar Outburst and Inner Disk Wall Destruction", The Astrophysical Journal, 978, 34.

Pascucci I, Beck T, Cabrit S, Bajaj N. S., Edwards S, Louvet F, Najita J, Skinner B, Gorti U, Salyk C, Brittain S, Krijt S, Muzerolle Page J, Ruaud M, Schwarz K, Semenov D, Duchêne G, Villenave M, 2024. "The nested morphology of disk winds from young stars revealed by JWST/NIRSpec observations", Nature Astronomy, 9, 81. 

Sellek A, Bajaj N. S., Pascucci I, Clarke C, Alexander R, Xie C, Ballabio G, Deng D, Gorti U, Gaspar A, Morrison J, 2024. "Modeling JWST MIRI-MRS Observations of T Cha: Mid-IR Noble Gas Emission Tracing a Dense Disk Wind", The Astronomical Journal, 167, 223.

Bajaj N. S., Pascucci I, Gorti U, Alexander R, Sellek A, Morrison J, Gaspar A, Clarke C, Xie C, Ballabio G, Deng D, 2024. "JWST MIRI MRS Observations of T Cha: Discovery of a Spatially Resolved Disk Wind", The Astronomical Journal, 167, 127.

Sandell, G., Reipurth, B., Vacca, W.D., and Bajaj, N.S., 2021. “FORCAST imaging of two small nearby Clusters: The Coronet and B59”, Astrophysical Journal, 920, 7

Bajaj, N.S., Patange, A.D., Jegadeeshwaran, R., Kulkarni, K.A., Ghatpande, R.S., and Kapadnis, A.M. 2022. "A Bayesian Optimized Discriminant Analysis Model for Condition Monitoring of Face Milling Cutter Using Vibration Datasets." ASME J Nondestructive Evaluation, ASME. 5(2): 021002

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