HST survey of the Orion Nebula Cluster in the H$_2$O 1.4 $\mu$m absorption band: I. A census of substellar and planetary mass objects

@article{Robberto2020HSTSO,
  title={HST survey of the Orion Nebula Cluster in the H\$_2\$O 1.4 \$\mu\$m absorption band: I. A census of substellar and planetary mass objects},
  author={M. Robberto and M. Gennaro and M. Gabellini and L. Hillenbrand and C. Pacifici and L. {\'U}beda and M. Andersen and T. Barman and A. Bellini and N. D. Rio and S. D. Mink and G. Lodato and C. Manara and I. Platais and L. Pueyo and G. Strampelli and J. Tan and L. Testi},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2020}
}
  • M. Robberto, M. Gennaro, +15 authors L. Testi
  • Published 2020
  • Physics
  • arXiv: Solar and Stellar Astrophysics
  • In order to obtain a complete census of the stellar and sub-stellar population, down to a few M$_{Jup}$ in the $\sim1$ Myr old Orion Nebula Cluster, we used the infrared channel of the Wide Field Camera 3 of the Hubble Space Telescope with the F139M and F130N filters. These bandpasses correspond to the $1.4 \mu$m H$_2$O absorption feature and an adjacent line-free continuum region. Out of $4,504$ detected sources, $3,352$ (about $75\%$) appear fainter than m$_{130}=14$ (Vega mag) in the F130N… CONTINUE READING
    3 Citations

    References

    SHOWING 1-10 OF 80 REFERENCES
    Protoplanetary Disks in the Orion OMC1 Region Imaged with ALMA
    • 28
    • PDF
    THE INITIAL MASS FUNCTION OF THE ORION NEBULA CLUSTER ACROSS THE H-BURNING LIMIT
    • 90
    • PDF
    Orion revisited - II. The foreground population to Orion A
    • 42
    • Highly Influential
    • PDF
    Constraints on the Stellar/Substellar Mass Function in the Inner Orion Nebula Cluster
    • 244
    • PDF
    Stellar rotation and variability in the Orion Nebula Cluster
    • 195
    • Highly Influential
    • PDF
    The Spectroscopically Determined Substellar Mass Function of the Orion Nebula Cluster
    • 152
    • PDF
    Hubble Space Telescope Measures of Mass Accretion Rates in the Orion Nebula Cluster
    • 47
    • PDF