Figure 6 from

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

TESS Hunt for Young and Maturing Exoplanets (THYME). IX. A 27 Myr Extended Population of Lower Centaurus Crux with a Transiting Two-planet System

Authors: Mackenna L. Wood, Andrew W. Mann, Madyson G. Barber, Jonathan L. Bush, Adam L. Kraus, Benjamin M. Tofflemire, Andrew Vanderburg, Elisabeth R. Newton, Gregory A. Feiden, George Zhou, Luke G. Bouma, Samuel N. Quinn, David J. Armstrong, Ares Osborn, Vardan Adibekyan, Elisa Delgado Mena, Sergio G. Sousa, Jonathan Gagné, Matthew J. Fields, Reilly P. Milburn, Pa Chia Thao, Stephen P. Schmidt, Crystal L. Gnilka, Steve B. Howell, Nicholas M. Law, Carl Ziegler, César Briceño, George R. Ricker, Roland Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Joshua E. Schlieder, Hugh P. Osborn, Joseph D. Twicken, David R. Ciardi, Chelsea X. Huang

Mackenna L. Wood et al 2023 The Astronomical Journal 165 .

Provider: AAS Journals

Caption: Figure 6.

The lithium-depletion boundary (LDB) of MELANGE-4. Shown is the color (J − K) and absolute magnitude (K _s) of members of MELANGE-4. Observed stars with EW(Li) > 300 mÅ are shown as colored dots, and stars with EW(Li) < 300 mÅ as red X’s. Candidate association members that were not observed are shown as gray dots. Orange and yellow lines show the predicted 20 and 30 Myr 99% LDBs using the DSEP magnetic models with two different solar abundances. The 30 Myr GS98 line has been moved up by 0.03 magnitudes to increase visibility. The solid black lines through the brightest M-dwarf with Li absorption, and the faintest likely member without Li absorption show the edges of the boundary region.

Copyright and Terms & Conditions

Additional terms of reuse

Other Images in This Article

Copyright and Terms & Conditions