output
19952026
most citedDigital Twin: Enabling Technologies, Challenges and Open Research

2.9k citations

Showing 2005 · astro-phShow all

27 papers · 2 filters

astro-ph2005★ 54 cited

An XMM-Newton observation of the young open cluster NGC 2547: coronal activity at 30 Myr

R. D. Jeffries, P. A. Evans, J. P. Pye +1

We report XMM-Newton observations of the young open cluster NGC 2547 which allow us to characterise coronal activity in solar-type stars at an age of 30 Myr. X-ray emission peaks a…

astro-ph2005

On the metallicity dependence of the winds from red supergiants and Asymptotic Giant Branch stars

Jacco Th. van Loon

Over much of the initial mass function, stars are destined to become luminous and cool red giants. They may then be able to produce dust in an atmosphere which has been elevated by…

astro-ph2005★ 55 cited

Stellar mass loss and the Intra-Cluster Medium in Galactic globular clusters: a deep radio survey for HI and OH

Jacco Th. van Loon, Snezana Stanimirovic, A. Evans +1

We present the results of a survey, the deepest to date, for HI emission at 21 cm and OH emission at 18 cm (lines at 1612, 1665, 1667 and 1720 MHz) in the direction towards the Gal…

astro-ph2005★ 6 cited

Massive star feedback - from the first stars to the present

Jorick S. Vink

The amount of mass loss is of fundamental importance to the lives and deaths of very massive stars, the input of chemical elements and momentum into the interstellar and intergalac…

astro-ph2005★ 10 cited

Close binary systems among very low mass stars and brown dwarfs

R. D. Jeffries, P. F. L. Maxted

Using Monte Carlo simulations and published radial velocity surveys we have constrained the frequency and separation (a) distribution of very low mass star (VLM) and brown dwarf (B…

astro-ph2005★ 56 cited

Very Large Telescope three micron spectra of dust-enshrouded red giants in the Large Magellanic Cloud

Jacco Th. van Loon, Jonathan R. Marshall, Martin Cohen +4

We present ESO/VLT spectra in the 2.9--4.1 micron range for a large sample of infrared stars in the Large Magellanic Cloud (LMC), selected on the basis of MSX and 2MASS colours to…