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

2.9k citations

Showing 2001Show all

19 papers · 1 filter

astro-ph2001★ 57 cited

Detection of negative superhumps in a LMXRB -- an end to the long debate on the nature of V1405 Aql (X1916-053)

A. Retter, Y. Chou, T. Bedding

The detection of two similar periodicities (3001 and 3028 s) in the light curve of V1405 Aql, a low mass X-ray Binary (LMXRB), has attracted the attention of many observers. Two ba…

astro-ph2001★ 60 cited

No disks around low-mass stars and brown dwarfs in the young sigma Orionis cluster?

J. M. Oliveira, R. D. Jeffries, M. J. Kenyon +2

We report on the analysis of 2MASS near-infrared data of a sample of low-mass stars and brown dwarfs in the sigma Orionis cluster. Youth and cluster membership have been spectrosco…

astro-ph2001

The host galaxy of GRB010222: The strongest damped Lyman-alpha system known

I. Salamanca, L. Kaper, P. M. Vreeswijk +6

Analysis of the absorption lines in the afterglow spectrum of the gamma-ray burst GRB010222 indicates that its host galaxy (at a redshift of z=1.476) is the strongest damped Lyman-…

astro-ph2001★ 17 cited

Understanding the LMXB X2127+119 in M15 I. X-ray eclipses and dips

Zach Ioannou, T. Naylor, A. P. Smale +2

We present X-ray observations of the high-inclination low-mass X-ray binary system X2127+119 (AC211) in the globular cluster M15 (NGC 7078). The observations consist of data acquir…

astro-ph2001

A spectroscopic survey of stars brighter than B=16.6 magnitude in omega Centauri

Jacco Th. van Loon

Using the 2dF multi-fibre instrument at the AAT, we have carried out a spectroscopic survey of over 1500 stars brighter than B=16.6 mag, which have been confirmed by the proper mot…

astro-ph2001★ 14 cited

A search for radio emission from Galactic supersoft X-ray sources

R. N. Ogley, S. Chaty, M. Crocker +5

We have made a deep search for radio emission from all the northern hemisphere supersoft X-ray sources using the VLA and MERLIN telescopes, at 5 and 8.4 GHz. Three previously undet…