Search Publications

Searching for Low-Mass Binary Companions in M35 Using the Fine Guidance Sensors of the Hubble Space Telescope
DOI: 10.1086/509804 Bibcode: 2007AJ....133..394M

Harrison, T. E.; McArthur, Barbara; McNamara, B. J.

The Hubble Space Telescope Fine Guidance Sensors data on 23 stars in the intermediate-age cluster M35 having B-V<0.5 (~F7 V) are analyzed to test whether binary periods, separations, and masses can be estimated by measuring periodic variations in the residuals of their internal proper motions. Of the 23 stars examined, 4 appear to possess a per…

2007 The Astronomical Journal
eHST 1
Dust Distribution in [WR] Planetary Nebulae: a Case of M2-43
Bibcode: 2007BaltA..16..151H

Szczerba, R.; Hajduk, M.; Gesicki, K.

Simultaneous presence of O- and C-rich molecules and/or dust is commonly known as mixed or dual chemistry. C-rich [WR] central stars show at the same time the presence of polycyclic aromatic hydrocarbons (PAHs) and crystalline silicates in their nebulae. We perform radiative transfer modeling of ISO spectrum for M2-43 to determine spatial location…

2007 Baltic Astronomy
eHST 1
Using XMM-Newton to measure the spectrum of the Vela pulsar and its phase variation
DOI: 10.1007/s10509-007-9303-4 Bibcode: 2007Ap&SS.308..601M

De Luca, Andrea; Caraveo, Patrizia A.; Manzali, Armando

We report on our analysis of two XMM-Newton observations of the Vela pulsar performed in December 2000 (total exposure time: 96.5 ks). We succeeded in resolving the pulsar spectrum from the surrounding bright nebular emission taking advantage both of the accurate calibration of the EPIC point spread function and of the Chandra/HRC surface brightne…

2007 Astrophysics and Space Science
XMM-Newton 1
Ultraviolet spectroscopy of Comet 9P/Tempel 1 with Alice/Rosetta during the Deep Impact encounter
DOI: 10.1016/j.icarus.2006.08.032 Bibcode: 2007Icar..191S.258F

Parker, Joel Wm.; Bertaux, Jean-Loup; Stern, S. Alan +5 more

We report on spectroscopic observations of periodic Comet 9P/Tempel 1 by the Alice ultraviolet spectrograph on the Rosetta spacecraft in conjunction with NASA's Deep Impact mission. Our objectives were to measure an increase in atomic and molecular emissions produced by the excavation of volatile sub-surface material. We unambiguously detected ato…

2007 Icarus
Rosetta 1
A near-ultraviolet view of the inner region of M 31 with the large binocular telescope
DOI: 10.1051/0004-6361:20078407 Bibcode: 2007A&A...476..193B

Pasian, F.; Fontana, A.; Grazian, A. +28 more

Aims:We present a 900 s, wide-field U image of the inner region of the Andromeda galaxy obtained during the commissioning of the blue channel of the Large Binocular Camera mounted on the prime focus of the Large Binocular Telescope.
Methods: Relative photometry and absolute astrometry of individual sources in the image was obtained along with …

2007 Astronomy and Astrophysics
eHST 1
Revised Periods for QS Geminorum and V367 Geminorum
DOI: 10.1086/516602 Bibcode: 2007PASP..119..274H

Brown, Peter J.; Hintz, Eric G.

We have examined the field around the variable stars QS Geminorum and V367 Geminorum. For the δ Scuti-type variable QS Gem, we determined a revised period of 0.1346116 days, which is close to the originally published period from Hipparcos. For the eclipsing system V367 Gem, we found a period of 0.6992285 days, which is substantially different from…

2007 Publications of the Astronomical Society of the Pacific
Hipparcos 1
Ultra-Low-Frequency Solar He II 30.4 nm Pulsations
DOI: 10.1086/522618 Bibcode: 2007ApJ...670.1414G

Didkovsky, L.; Judge, D. L.; Gangopadhyay, P. +2 more

Solar EUV and X-ray measurements from the Charge, Element and Isotope Analysis System/Solar EUV Monitor (CELIAS/SEM) on board Solar and Heliospheric Observatory (SOHO) and the Geostationary Operational Environmental Satellites (GOES) have been studied for four time periods. Two ultra-low-frequency CELIAS/SEM He II 30.4 nm pulsations were observed …

2007 The Astrophysical Journal
SOHO 1
Stellar population in bulge of spiral galaxies
DOI: 10.1393/ncb/i2008-10492-y Bibcode: 2007NCimB.122.1281M

Saglia, R. P.; Morelli, L.; Corsini, E. M. +6 more

We present a preliminary analysis of ASTRO-F data of a complete sample of ~150 EROs (R-K>5) down to K(Vega)<19, for which reliable photometric redshifts are available, in the range 0.8<z<2, selected over two fields (S7 and S2) of the MUNICS survey. The area covered is about 420 arcmin^2. We have imaged this area with AKARI telescope in…

2007 Nuovo Cimento B Serie
AKARI 1
X-ray emission of OH megamaser galaxies
DOI: 10.1007/s10511-007-0014-x Bibcode: 2007Ap.....50..135K

Hambaryan, V. V.; Kandalyan, R. A.; Sabat, H. A.

The properties of OH megamaser galaxies in the x-ray region are discussed. Observational data from the XMM-Newton x-ray satellite are presented for three megamasers, IRAS 01418+1651, IRAS 11010+4107, and IRAS 13218+0552. Based on a sample of OH megamaser galaxies it is shown that the x-ray and OH emission are closely coupled. Megamaser emission al…

2007 Astrophysics
XMM-Newton 1
Evolution of coronal mass ejections in the early stage
DOI: 10.1016/j.asr.2007.02.055 Bibcode: 2007AdSpR..39.1847B

Zhang, Hongqi; Lin, Jun; Li, Leping +2 more

This work reports the investigation of two coronal mass ejections (CME) observed in white light, Hα, EUV and X-ray by various instruments both in space and on ground on February 18, 2003 and January 19, 2005, respectively. The white light coronal images show that the first CME began with the rarefaction of a region above the solar limb and was fol…

2007 Advances in Space Research
SOHO 1