activity
19962019
most citedSurface magnetic fields on two accreting T Tauri stars: CV Cha and CR Cha

106 citations · 1.7k across the 38 of their papers we have counts for

collaborators

38 papers

astro-ph.SR2019★ 11 cited

THOR 42: A touchstone 24 Myr-old eclipsing binary spanning the fully-convective boundary

Simon J. Murphy, Warrick A. Lawson, Christopher A. Onken +7

We present the characterization of CRTS J055255.7004426 (=THOR 42), a young eclipsing binary comprising two pre-main sequence M dwarfs (combined spectral type M3.5). This nearby…

astro-ph.SR2016★ 20 cited

Absorption at 11 microns in the interstellar medium and embedded sources: evidence for crystalline silicates

Christopher M Wright, Tho Do Duy, Warrick Lawson

An absorption feature is occasionally reported around 11 microns in astronomical spectra, including those of forming stars. Candidate carriers include water ice, polycyclic aromati…

astro-ph.SR2015★ 24 cited

New members of the TW Hydrae Association and two accreting M-dwarfs in Scorpius-Centaurus

Simon J. Murphy, Warrick A. Lawson, Joao Bento

We report the serendipitous discovery of several young mid-M stars found during a search for new members of the 30-40 Myr-old Octans Association. Only one of the stars may be consi…

astro-ph.SR2014★ 61 cited

New low-mass members of the Octans stellar association and an updated 30-40 Myr lithium age

Simon J. Murphy, Warrick A. Lawson

The Octans association is one of several young stellar moving groups recently discovered in the Solar neighbourhood, and hence a valuable laboratory for studies of stellar, circums…

astro-ph.SR2013★ 98 cited

Re-examining the membership and origin of the Epsilon Cha association

Simon J. Murphy, Warrick A. Lawson, Michael S. Bessell

We present a comprehensive investigation of the Epsilon Chamaeleontis association (Epsilon Cha), one of several young moving groups spread across the southern sky. We re-assess the…

astro-ph.SR2013★ 11 cited

Reverse dynamical evolution of Eta Chamaeleontis

Christophe Becker, Estelle Moraux, Gaspard Duchêne +2

In the scope of the star formation process, it is unclear how the environment shapes the initial mass function (IMF). While observations of open clusters propose a universal pictur…