Optical and NIR studies of short period low mass X-ray binaries (LMXB)
Not Available
Hakala, P. et al.
Advertised on:
11
2009
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Optical follow-up of ROSAT discovered candidate members of the open cluster Coma BerenicesWe have carried out an optical follow-up of twelve ROSAT discovered candidate members of the Coma Berenices open cluster. VRI photometry and low resolution ( ~ 3 Å) spectroscopy in the range 3800-7000 Åwere performed to obtain colour-magnitude diagrams, proper motions, spectral types, chromospheric activity levels and radial velocities that allowGarcía López, R. J. et al.
Advertised on:
112000 -
Optical Linear Polarization in the Case of Two Supernovae Associated to X-ray Flashes: XRF060218/SN2006aj and XRF080109/SN2008DWe present the polarization monitoring carried out for two SNe associated with GRBs: XRF060218/SN2006aj and XRF080109/SN2008D. For XRF060218/SN2006aj we measured a mean polarization of P˜4% at 2.6-5.6 days after the X-ray event. This is the highest polarization value ever measured for a supernova. We derived the intrinsic polarization of XRF080109Gorosabel, J. et al.
Advertised on:
112011 -
Optical novae: the major class of supersoft X-ray sources in M 31We searched for X-ray counterparts of optical novae detected in M 31 and M 33. We combined an optical nova catalogue from the WeCAPP survey with optical novae reported in the literature and correlated them with the most recent X-ray catalogues from ROSAT, XMM-Newton, and Chandra, and in addition searched for nova correlations in archival data. WePietsch, W. et al.
Advertised on:
112005 -
Optical studies of V404 Cyg, the X-ray transient GS 2023+338. IV. The rotation speed of the companion star.Not AvailableCasares, J. et al.
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111994 -
Optical variability of the ultracool dwarf TVLM 513-46546: evidence for inhomogeneous dust cloudsWe present multicolour photometry of the M8.5V ultracool dwarf `pulsar' TVLM 513-46546 (hereafter TVLM 513) obtained with the triple-beam photometer ULTRACAM. Data were obtained simultaneously in the Sloan-g' and Sloan-i' bands. The previously reported sinusoidal variability, with a period of 2 h, is recovered here. However, the Sloan-g' and SloanLittlefair, S. P. et al.
Advertised on:
112008