Search Publications

X-ray properties of active M dwarfs as observed by XMM-Newton
DOI: 10.1051/0004-6361:20041941 Bibcode: 2005A&A...435.1073R

Schmitt, J. H. M. M.; Robrade, J.

We present a comparative study of X-ray emission from a sample of active M dwarfs with spectral types using XMM-Newton observations of two single stars, AD Leonis and EV Lacertae, and two unresolved binary systems, AT Microscopii and EQ Pegasi. The light curves reveal frequent flaring during all four observations. We perform a uniform spectral ana…

2005 Astronomy and Astrophysics
XMM-Newton 75
A search for changing-look AGN in the Grossan catalog
DOI: 10.1051/0004-6361:20053389 Bibcode: 2005A&A...442..185B

Maiolino, R.; Fiore, F.; Bianchi, S. +4 more

We observed with XMM-Newton 4 objects selected from the Grossan (1992, Ph.D. Thesis) catalog, with the aim to search for new "changing-look" AGN. The sample includes all the sources which showed in subsequent observations a flux much lower than the one measured with HEAO A-1: NGC 7674, NGC 4968, IRAS 13218+0552 and NGC 1667. None of the sources wa…

2005 Astronomy and Astrophysics
XMM-Newton 75
Submillimetre photometry of X-ray absorbed quasi-stellar objects: their formation and evolutionary status
DOI: 10.1111/j.1365-2966.2005.09051.x Bibcode: 2005MNRAS.360..610S

Ivison, R. J.; Smail, Ian; Page, M. J. +4 more

We present an analysis of the submillimetre/X-ray properties of 19 X-ray absorbed, Compton-thin quasi-stellar objects (QSOs) selected to have luminosities and redshifts that represent the peak of cosmic QSO activity, i.e. ~L* objects at 1 < z < 3. Of these, we present new data for 11 objects not previously observed at submillimetre wavelengt…

2005 Monthly Notices of the Royal Astronomical Society
XMM-Newton 75
A Wide-Field Hubble Space Telescope Survey of the Cluster Cl 0024+16 at z = 0.4. III. Spectroscopic Signatures of Environmental Evolution in Early-Type Galaxies
DOI: 10.1086/497024 Bibcode: 2005ApJ...634..977M

Smith, Graham P.; Treu, Tommaso; Smail, Ian +4 more

We report results from a panoramic spectroscopic survey of 955 objects in the field of the rich cluster Cl 0024+1654 (z~=0.4), complementing the HST imaging presented in the first paper in this series. Combining with previous work, we compile a catalog of 1394 unique redshifts in the field of this cluster, including 486 cluster members spread acro…

2005 The Astrophysical Journal
eHST 75
8-13 µm Spectroscopy of Young Stellar Objects: Evolution of the Silicate Feature
DOI: 10.1086/427793 Bibcode: 2005ApJ...622..404K

Meyer, Michael R.; Hillenbrand, Lynne A.; Blake, Geoffrey A. +1 more

Silicate features arising from material around pre-main-sequence stars are useful probes of the star and planet formation process. In order to investigate possible connections between dust processing and disk properties, 8-13 µm spectra of 34 young stars, exhibiting a range of circumstellar environments and including spectral types A-M, were…

2005 The Astrophysical Journal
ISO 75
Complex X-Ray Absorption and the Fe Kα Profile in NGC 3516
DOI: 10.1086/425961 Bibcode: 2005ApJ...618..155T

Turner, T. J.; Kraemer, S. B.; Reeves, J. N. +2 more

We present data from simultaneous Chandra, XMM-Newton, and BeppoSAX observations of the Seyfert 1 galaxy NGC 3516, taken during 2001 April and November. We have investigated the nature of the very flat observed X-ray spectrum. Chandra grating data show the presence of X-ray absorption lines, revealing two distinct components of the absorbing gas, …

2005 The Astrophysical Journal
XMM-Newton eHST 75
Self-Consistent Magnetohydrodynamic Modeling of a Coronal Mass Ejection, Coronal Dimming, and a Giant Cusp-shaped Arcade Formation
DOI: 10.1086/496943 Bibcode: 2005ApJ...634..663S

Shibata, Kazunari; Chen, P. F.; Isobe, Hiroaki +3 more

We performed magnetohydrodynamic simulations of coronal mass ejections (CMEs) and associated giant arcade formations, and the results suggest new interpretations of observations of CMEs. We performed two cases of the simulation: with and without heat conduction. Comparing between the results of the two cases, we found that the reconnection rate in…

2005 The Astrophysical Journal
SOHO 74
Multifractal Analysis Of Solar Magnetograms
DOI: 10.1007/s11207-005-3525-9 Bibcode: 2005SoPh..228...29A

Abramenko, Valentyna I.

As solar observational techniques improve, fine small-scale structures observed on the solar surface become more pronounced. Complex filigree structures of solar granulation, sunspots, photospheric magnetic and velocity fields cannot be described adequately by a single parameter (e.g., filling factor, fractal dimension, or power-law index). Method…

2005 Solar Physics
SOHO 74
The WEBT campaign to observe AO 0235+16 in the 2003-2004 observing season. Results from radio-to-optical monitoring and XMM-Newton observations
DOI: 10.1051/0004-6361:20042567 Bibcode: 2005A&A...438...39R

Lähteenmäki, A.; Papadakis, I. E.; Smith, N. +64 more

A multiwavelength campaign to observe the BL Lac object AO 0235+16 (z=0.94) was set up by the Whole Earth Blazar Telescope (WEBT) collaboration during the observing seasons 2003-2004 and 2004-2005, involving radio, near-IR and optical photometric monitoring, VLBA monitoring, optical spectral monitoring, and three pointings by th…

2005 Astronomy and Astrophysics
XMM-Newton 74
The NGC 5846 Group: Dynamics and the Luminosity Function to MR=-12
DOI: 10.1086/444560 Bibcode: 2005AJ....130.1502M

Mahdavi, Andisheh; Tully, R. Brent; Trentham, Neil

We conduct a photometric and spectroscopic survey of a 10 deg2 region surrounding the nearby NGC 5846 group of galaxies, using the Canada-France-Hawaii and Keck I telescopes to study the population of dwarf galaxies as faint as MR=-10. Candidates are identified on the basis of quantitative surface brightness and qualitative m…

2005 The Astronomical Journal
XMM-Newton 74