Search Publications

Response of Hinode XRT to quiet Sun, active region and flare plasma
DOI: 10.1051/0004-6361/201016346 Bibcode: 2014A&A...561A..20O

Mason, H. E.; Del Zanna, G.; O'Dwyer, B.


Aims: We examine the response of the Hinode X-Ray Telescope (XRT), using simultaneous observations with the Hinode Extreme-ultraviolet Imaging Spectrometer (EIS), for a flare, an active region and a quiet Sun region. We also examine the relative intensity calibration of EIS and XRT.
Methods: EIS differential emission measure distribution…

2014 Astronomy and Astrophysics
Hinode 11
Astrometry of χ and H Persei Based on Processing of Digitized Plates of Archive of the Astronomical Institute of the Academy of Sciences of the Republic of Uzbekistan
Bibcode: 2014OAP....27...57M

Ehgamberdiev, Sh. A.; Muminov, M. M.; Yuldoshev, Q. X. +3 more

Work is done with Epson Expression 10000XL scanner of Astronomical Institute (AI) of the Academy of Sciences of Uzbekistan. The plates were exposed with the Normal astrograph (D/F = 330mm / 3467mm, M = 59.56"/mm). The digitization of plates with (16x16) cm in size was made with resolution of 1200 dpi (1px = 1.25"). Test research was done using pla…

2014 Odessa Astronomical Publications
Hipparcos 11
Broad iron emission line and kilohertz quasi-periodic oscillations in the neutron star system 4U 1636-53
DOI: 10.1093/mnras/stu490 Bibcode: 2014MNRAS.440.3275S

Hiemstra, Beike; Belloni, Tomaso; Méndez, Mariano +3 more

Both the broad iron (Fe) line and the frequency of the kilohertz quasi-periodic oscillations (kHz QPOs) in neutron star low-mass X-ray binaries (LMXBs) can potentially provide independent measures of the inner radius of the accretion disc. We use XMM-Newton and simultaneous Rossi X-ray Timing Explorer observations of the LMXB 4U 1636-53 to test th…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 11
Herschel/PACS observations of the host galaxy of GRB 031203.
DOI: 10.1093/mnrasl/slu090 Bibcode: 2014MNRAS.443L.124S

Page, M. J.; Symeonidis, M.; Schady, P. +6 more

We present Herschel/PACS observations of the nearby (z = 0.1055) dwarf galaxy that has hosted the long gamma-ray burst (LGRB) 031203. Using the PACS data, we have been able to place constraints on the dust temperature, dust mass, total infrared (IR) luminosity and IR-derived star formation rate (SFR) for this object. We find that the GRB host gala…

2014 Monthly Notices of the Royal Astronomical Society
Herschel 11
Multi-frequency study of DEM L299 in the Large Magellanic Cloud
DOI: 10.1051/0004-6361/201423575 Bibcode: 2014A&A...567A.136W

Sasaki, Manami; Warth, Gabriele; Filipović, Miroslav D. +3 more


Aims: We have studied the H ii region DEM L299 in the Large Magellanic Cloud (LMC) to understand its physical characteristics and morphology in different wavelengths.
Methods: We performed a spectral analysis of archived XMM-Newton EPIC data and studied the morphology of DEM L299 in X-ray, optical, a…

2014 Astronomy and Astrophysics
XMM-Newton 11
Chandra X-ray observation of the H ii region Gum 31 in the Carina nebula complex
DOI: 10.1051/0004-6361/201323133 Bibcode: 2014A&A...564A.120P

Preibisch, T.; Ratzka, T.; Broos, P. +2 more

Context. Gum 31 is a prominent, but still rather poorly studied H ii region around the stellar cluster NGC 3324 at the northwestern periphery of the Carina nebula complex.
Aims: Our aim was to reveal and characterize the young stellar population in Gum 31. An X-ray survey is the only efficient way to identify young stars in this region with e…

2014 Astronomy and Astrophysics
eHST 11
How to distinguish between kink and sausage modes in flapping oscillations?
DOI: 10.1002/2013JA019477 Bibcode: 2014JGRA..119.3002K

Kubyshkin, I. V.; Sergeev, V. A.; Semenov, V. S. +5 more

Flapping waves are most noticeable large-scale perturbations of the magnetotail current sheet, whose nature is still under discussion. They represent rather slow (an order of magnitude less than typical Alfven speed) waves propagating from the center of the sheet to its flanks with a typical speed of 20-60 km/s, amplitude of 1-2 Re and …

2014 Journal of Geophysical Research (Space Physics)
Cluster 11
Absorption features in the quasar HS 1603 + 3820 II. Distance to the absorber obtained from photoionisation modelling
DOI: 10.1016/j.newast.2013.08.009 Bibcode: 2014NewA...28...70R

Różańska, A.; Hryniewicz, K.; Ebeling, H. +4 more

We present the photoionisation modelling of the intrinsic absorber in the bright quasar HS 1603 + 3820. We constructed the broad-band spectral energy distribution using the optical/UV/X-ray observations from different instruments as inputs for the photoionisation calculations. The spectra from the Keck telescope show extremely high CIV to HI ratio…

2014 New Astronomy
IUE 11
The innermost globular clusters of M87
DOI: 10.1093/mnras/stu948 Bibcode: 2014MNRAS.442.1350M

Prieto, M. A.; Acosta-Pulido, J. A.; Fernández-Ontiveros, J. A. +1 more

We present a comprehensive multiwavelength photometric analysis of the innermost (∼3 × 3 kpc2) 110 globular clusters (GCs) of M87. Their spectral energy distributions (SEDs) were built taking advantage of new ground-based high-resolution near-infrared imaging aided by adaptive optics at the Very Large Telescope combined with Hubble Spac…

2014 Monthly Notices of the Royal Astronomical Society
eHST 11
Weighing Neutrinos in f(R) Gravity in Light of BICEP2
DOI: 10.1088/0253-6102/62/1/18 Bibcode: 2014CoTPh..62..102Z

Zhou, Xiao-Ying; He, Jian-Hua

We constrain the neutrino mass in f(R) gravity using the latest observations from the Planck, BAO and BICEP2 data. We find that the measurement on the B-modes can break the degeneracy between the massive neutrinos and the f(R) gravity. We find a non-zero value of the Compton wavelengths B0 at a 68% confidence level for the f(R) model in…

2014 Communications in Theoretical Physics
Planck 11