Search Publications

HD 143418: an unusual light variable and a double-lined spectroscopic binary with a CP primary
DOI: 10.1051/0004-6361:20042546 Bibcode: 2007A&A...464..263B

Wolf, M.; Prša, A.; Harmanec, P. +7 more

Aims:After a serendipitious discovery that HD 143418 is a light variable, we analyzed numerous UB{}V observations and Hipparcos Hp magnitudes transformed to Johnson V to find out whether the object is a very unusual spectroscopic binary.
Methods: Initial reductions of new photometry were carried out with the HEC22 program, while the…

2007 Astronomy and Astrophysics
Hipparcos 5
EROs found behind lensing clusters. I. Stellar populations and dust properties of optical dropout EROs and comparison with related objects
DOI: 10.1051/0004-6361:20077127 Bibcode: 2007A&A...469...47S

Kneib, J. -P.; Schaerer, D.; Pelló, R. +6 more

Context: On the nature, redshift, stellar populations and dust properties of optically faint or non-detected extremely red objects.
Aims: Determining the nature, redshift, stellar populations and dust properties of optically faint or non-detected, extremely red objects (ERO) found from our survey of the lensing clusters A1835 and AC114 (Richar…

2007 Astronomy and Astrophysics
eHST 5
CCD astrometry and components instrumental magnitude difference of 432 Hipparcos wide visual double stars
DOI: 10.1051/0004-6361:20066290 Bibcode: 2007A&A...472.1055S

Gavras, P.; Sinachopoulos, D.; Dionatos, O. +2 more

Context: We measured the angular separations, position angles, Δ V, Δ y and Δ I of wide visual double stars during the period 2003-2005. At least one component of the double stars in our sample has an entry in the Hipparcos catalogue.
Aims: Our measurements are a contribution to the study of the nature of these double stars.
Methods: The n…

2007 Astronomy and Astrophysics
Hipparcos 5
INTEGRAL high energy detection of the transient IGR J11321-5311
DOI: 10.1051/0004-6361:20077439 Bibcode: 2007A&A...468L..21S

Hill, A. B.; Bird, A. J.; Ubertini, P. +5 more

Context: The transient hard X-ray source IGR J11321-5311 was discovered by INTEGRAL on June 2005, during observations of the Crux spiral arm. To date, this is the only detection of the source to be reported by any X/γ-ray mission.
Aims: To characterize the behaviour and hence the nature of the source through temporal and spectral IBIS analysis…

2007 Astronomy and Astrophysics
INTEGRAL 5
Coronal mass ejections and the associated activities on the solar disk observed on October 26, 2003
DOI: 10.1051/0004-6361:20065471 Bibcode: 2007A&A...463..321B

Zhang, H.; Lin, J.; Stenborg, G. A. +1 more

Aims:Coronal mass ejections (CMEs) are usually considered fast (slow) if their velocities are greater (less) than 500 km s-1. It is generally believed that fast CMEs are well associated with activity manifested on the solar disk, such as solar flares, and that slow CMEs are often associated with filament eruptions out of active regions …

2007 Astronomy and Astrophysics
SOHO 4
The nearby QSO host I Zw 1: the stellar disk and adjacent objects
DOI: 10.1051/0004-6361:20066359 Bibcode: 2007A&A...469..913S

Saviane, I.; Scharwächter, J.; Eckart, A. +2 more

Context: The relation between tidal interactions, starbursts, and the onset and/or fueling of active galactic nuclei (AGN) is a matter of debate. I Zw 1 is considered as the prototypical narrow-line Seyfert 1 galaxy (NLS1) and as one of the closest quasi-stellar objects (QSOs). With a clear spiral host and a small companion gala…

2007 Astronomy and Astrophysics
eHST 4
The in-flight monitoring and validation of the SOHO CDS Normal Incidence Spectrometer radiometric calibration
DOI: 10.1051/0004-6361:20054477 Bibcode: 2007A&A...463..339L

Lanzafame, A. C.; Brooks, D. H.; Thompson, W. T. +3 more

The scientific return from an extreme-ultraviolet spectrometer depends on the accuracy and precision of its radiometric calibration. For the Coronal Diagnostic Spectrometer on SOHO, radiometric calibration started pre-launch in the laboratory and continued after launch by making comparison measurements of the same area of the Sun with calibrated s…

2007 Astronomy and Astrophysics
SOHO 4
ISOCAM mid-infrared spectroscopy and NIR photometry of the HII complex N4 in the Large Magellanic Cloud
DOI: 10.1051/0004-6361:20066587 Bibcode: 2007A&A...469..539C

Boulanger, F.; Sauvage, M.; Contursi, A. +3 more

Context: We present the analysis of ISOCAM-CVF and the J, H, and Ks photometry data for the HII region complex N4 in the Large Magellanic Cloud (LMC).
Aims: The aim is twofold: 1) to study the connection between the interstellar medium and the star content of this region; 2) to investigate the effects of the lower-than-Galactic meta…

2007 Astronomy and Astrophysics
ISO 4
An XMM-Newton view of the X-ray flat radio-quiet quasar PG 1416-129
DOI: 10.1051/0004-6361:20066048 Bibcode: 2007A&A...466...23P

Nandra, K.; Turner, T. J.; Porquet, D. +3 more

Aims:The radio-quiet quasar PG 1416-129 (z=0.129) exhibits atypical optical and X-ray properties. Between 1990 and 2000, in response to its optical continuum decrease, the “classical” broad component of Hβ almost completely disappeared, with a factor of 10 decrease in the line flux. In addition, the width of the broad component of the Hβ line decr…

2007 Astronomy and Astrophysics
XMM-Newton 4
X-ray detection of the substellar twin 2MASS J11011926-7732383 AB
DOI: 10.1051/0004-6361:20077564 Bibcode: 2007A&A...474..129S

Micela, G.; Stelzer, B.

Context: 2MASS J11011926-7732383 AB (hereafter 2M 1101 AB), located in the Cha I star forming region, is a rare wide-separation brown dwarf binary. Being spatially resolvable in many wavebands, it is a unique target for studying the properties of substellar twins.
Aims: Here, we exploit the coeval pair 2M 1101 AB to examine the influence of ph…

2007 Astronomy and Astrophysics
XMM-Newton 4