output
19952026
most citedUniaxial Strain in Graphene by Raman Spectroscopy: G peak splitting, Gruneisen Parameters and Sample Orientation

2k citations

Showing 2000 · astro-phShow all

7 papers · 2 filters

astro-ph2000★ 43 cited

Comparison of the H-alpha circumstellar disks in Be/X-ray binaries and Be stars

R. K. Zamanov, P. Reig, J. Marti +4

We present a comparative study of the circumstellar disks in Be/X-ray binaries and isolated Be stars based upon the H-alpha emission line. From this comparison it follows that the…

astro-ph2000★ 4 cited

Optical and X-ray monitoring of the NLS1 galaxy Ark 564

I. E. Papadakis, W. Brinkmann, H. Negoro +3

The Narrow-line Seyfert galaxy Ark 564 was monitored between June 04, 2000 and June 24, 2000 from Skinakas Observatory. The B,V,R and I band light curves show night to night variat…

astro-ph2000★ 29 cited

The Be/X-ray binary LS 992/RX J0812.4-3114: physical parameters and long-term variability

P. Reig, I. Negueruela, D. A. H. Buckley +3

We present the first long-term optical and infrared study of the optical counterpart to the source RX J0812.4-3114, an X-ray pulsar with a Be type companion. During the period cove…

astro-ph2000★ 24 cited

Deep Halpha imagery of the Eridanus shells

P. Boumis, C. Dickinson, J. Meaburn +5

A deep \ha image of interlocking filamentary arcs of nebulosity has been obtained with a wide-field ( 30\degree diameter) narrow-band filter camera combined with a CCD as…

astro-ph2000★ 21 cited

Correlated V/R and IR photometric variations in the Be/X-ray binary LS I +61 235/RX J0146.9+6121

P. Reig, I. Negueruela, M. J. Coe +3

We report on the long-term variability of the Be/X-ray binary LS I +61 235/RX J0146.9+6121. New optical spectroscopic and infrared photometric observations confirm the presence of…

astro-ph2000★ 1 cited

Dust properties of external galaxies; NGC 891 revisited

P. B. Alton, E. M. Xilouris, S. Bianchi +2

We compare 850um SCUBA images of NGC 891 with the corresponding V-band optical depth predicted from radiation transfer simulations. These two tracers of dust show a very similar di…