activity
19992025
most citedThe XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

372 citations · 1k across the 33 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR20253 cited

Substellar Initial Mass Function of Trumpler 14

Tamara Rom, Estelle Moraux, Koraljka Mužić +3

Young, massive stellar clusters offer a prime setting to explore brown dwarf (BD) formation under high densities and intense UV radiation. Trumpler 14 (Tr 14), a 1 Myr-old cluster…

astro-ph.SR202129 cited

The HD 98800 quadruple pre-main sequence system. Towards full orbital characterisation using long-baseline infrared interferometry

S. Zúñiga-Fernández, J. Olofsson, A. Bayo +8

HD 98800 is a young ( Myr old) and nearby ( pc) quadruple system, composed of two spectroscopic binaries orbiting around each other (AaAb and BaBb), with a gas-rich…

astro-ph.SR202118 cited

A MUSE Spectro-imaging Study of the Th 28 Jet: Precession in the Inner Jet

A. Murphy, C. Dougados, E. T. Whelan +5

Context: Th 28 is a Classical T Tauri star in the Lupus 3 cloud which drives an extended bipolar jet. Previous studies of the inner jet identified signatures of rotation around the…

astro-ph.SR202113 cited

Resolving the dynamical mass tension of the massive binary 9 Sagittarii

M. Fabry, C. Hawcroft, A. J. Frost +4

Direct dynamical mass measurements of stars with masses above 30 M are rare. This is the result of the low yield of the upper initial mass function and the limited number…

astro-ph.SR20174 cited

The wind and the magnetospheric accretion onto the T Tauri star S Coronae Australis at sub-au resolution

R. Garcia Lopez, K. Perraut, A. Caratti o Garatti +70

To investigate the inner regions of protoplanetary disks, we performed near-infrared interferometric observations of the classical TTauri binary system S CrA. We present the first…

astro-ph.SR20091 cited

Multi-wavelength observing of a forming solar-like star

S. G. Gregory, E. Flaccomio, C. Argiroffi +7

V2129 Oph is a 1.35 solar mass classical T Tauri star, known to possess a strong and complex magnetic field. By extrapolating from an observationally derived magnetic surface map,…