Pulsars, transients and relativistic astrophysics

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On the Nature of XTE J0421+560/CI Camelopardalis

The Astrophysical Journal American Astronomical Society 527:1 (1999) 345-352

Authors:

T Belloni, S Dieters, ME van den Ancker, RP Fender, DW Fox, BA Harmon, M van der Klis, JM Kommers, WHG Lewin, J van Paradijs
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The Bulge Globular Cluster NGC 6553: Observations with HST's WFPC2, STIS, and NICMOS

(1999)

Authors:

Sylvie F Beaulieu, Gerard F Gilmore, Rachel A Johnson, Stephen J Smartt, Nial Tanvir, Basilio Santiago
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Near IR spectroscopy of candidate B[e]/X-ray binaries

Astronomy and Astrophysics 348:3 (1999) 888-896

Authors:

JS Clark, IA Steele, RP Fender, MJ Coe

Abstract:

We present near TR spectra (0.8-2.5 μm) of the two candidate B[e]/X-ray binary systems CI Cam/XTE J0421+560 and HD34921/1H 0521+37. The spectra of both systems show evidence for a more complex circumstellar environment than those seen in classical Be/X-ray binaries. Strong H I and He I emission is seen, confirming the presence of a dense circumstellar wind; O I, Fe II and [Fe II] emission in CI Cam points to recombination of this wind. He II emission, presumably due to excitation by the compact companion is observed in CI Cam. Finally, emission is seen from Na I and CO, which implies regions of the circumstellar environment with much lower excitation temperatures and higher densities, shielded from direct stellar radiation. Both systems show evidence for continuum emission from circumstellar dust. Neither of these two features has previously been observed in any other classical Be/X-ray binary system. Adopting the classification criteria of Lamers et al. (1998) we suggest identifications of unclB[e] and sgB[e] for HD34921 and CI Cam respectively, making them the first High Mass X-ray Binaries with primaries showing the B[e] phenomenon known.

Transport in accretion disks

Physics of Plasmas AIP Publishing 6:12 (1999) 4444-4449

Authors:

John F Hawley, Steven A Balbus
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VLT FORS spectra of blue supergiants in the Local Group galaxy NGC 6822

Astronomy and Astrophysics 352:1 (1999)

Authors:

B Muschielok, RP Kudritzki, I Appenzeller, F Bresolin, K Butler, W Gässier, R Häfner, HJ Hess, W Hummel, DJ Lennon, KH Mantel, W Meisl, W Seifert, SJ Smartt, T Szeifert, K Tarantik

Abstract:

Half hour exposures using the ESO VLT/FORS1 combination at Parañal in Chile have allowed us to obtain spectra for three B supergiants in the dwarf irregular galaxy NGC 6822. The spectra have been analysed using non-LTE techniques and temperatures, gravities, helium content and abundances have been obtained. Overall the metallicity of NGC 6822 is found to lie between that of the LMC and of the SMC, in agreement with previous observations of H II regions and in contrast to the earlier findings of Massey et al. (1995). The analysis of Hα yields estimates of the mass-loss rates and wind momenta. These results demonstrate that significantly longer exposures with the same instruments will allow us to perform quantitative spectroscopy of blue supergiants in galaxies far beyond the Local Group.