Search Publications

Evaluation of In-Orbit Thermal Performance of X-Ray Astronomy Satellite ``Hitomi''
DOI: 10.2514/1.A33903 Bibcode: 2018JSpRo..55...77I

Kokubun, Motohide; Takahashi, Tadayuki; Takei, Yoh +7 more

2018 Journal of Spacecraft and Rockets
Hitomi 5
Phase-dependent Photometric and Spectroscopic Characterization of the MASTER-Net Optical Transient J212444.87+321738.3: An Oxygen-rich Mira
DOI: 10.3847/1538-3881/aab902 Bibcode: 2018AJ....155..216G

Banerjee, D. P. K.; Hambsch, Franz-Josef; Dutta, Somnath +4 more

We describe the time-dependent properties of a new spectroscopically confirmed Mira variable, which was discovered in 2013 as MASTER-Net Optical Transient J212444.87+321738.3 toward the Cygnus constellation. We have performed long-term optical/near-infrared (NIR) photometric and spectroscopic observations to characterize the object. From the optic…

2018 The Astronomical Journal
AKARI 5
An ultraviolet study of B[e] stars: evidence for pulsations, luminous blue variable type variations and processes in envelopes
DOI: 10.1093/mnras/sty749 Bibcode: 2018MNRAS.477..236K

Krtička, J.; Krtičková, I.

Stars that exhibit a B[e] phenomenon comprise a very diverse group of objects in a different evolutionary status. These objects show common spectral characteristics, including the presence of Balmer lines in emission, forbidden lines and strong infrared excess due to dust. Observations of emission lines indicate illumination by an ultraviolet ioni…

2018 Monthly Notices of the Royal Astronomical Society
IUE 5
Dwarf irregular galaxy Leo A extends even farther, according to HST WFC3 photometry
DOI: 10.1051/0004-6361/201731840 Bibcode: 2018A&A...614A.144S

Vansevičius, V.; Stonkutė, R.; Čeponis, M. +2 more

Context. Leo A is an isolated gas-rich dwarf irregular galaxy of low stellar mass and metallicity residing at the outskirts of the Local Group. Ages of the stellar populations in Leo A range from 10 Myr to 10 Gyr. A large stellar halo (up to the deprojected distance of 1.7 kpc) was discovered based on Subaru wide-field photometry of red giant bran…

2018 Astronomy and Astrophysics
eHST 5
Astrometric Observations of the Galilean Moons of Jupiter at the Pulkovo Normal Astrograph in 2016-2017
DOI: 10.1134/S0038094618040020 Bibcode: 2018SoSyR..52..312N

Khovrichev, M. Yu.; Narizhnaya, N. V.; Apetyan, A. A. +6 more

We present the results of observations of the Galilean moons of Jupiter carried out at the Normal Astrograph of the Pulkovo Observatory in 2016-2017. We obtained 761 positions of the Galilean moons of Jupiter in the system of the Gaia DR1 catalog (ICRF, J2000.0) and 854 differential coordinates of the satellites relative to each other. The mean er…

2018 Solar System Research
Gaia 5
A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart
DOI: 10.1093/mnras/sty2387 Bibcode: 2018MNRAS.481.1416S

Sezer, A.; Yamazaki, R.; Ergin, T. +2 more

Kes 69 is a mixed-morphology (MM) supernova remnant (SNR) that is known to be interacting with molecular clouds based on 1720 MHz hydroxyl (OH) maser emission observations in the northeastern and southeastern regions. We present an investigation of Kes 69 using ∼67 ks Suzaku observation. The X-ray spectrum of the whole SNR is well fitted by a non-…

2018 Monthly Notices of the Royal Astronomical Society
Suzaku 5
Added-value interfaces to asteroid photometric and spectroscopic data in the Gaia database
DOI: 10.1016/j.asr.2018.04.035 Bibcode: 2018AdSpR..62..464T

Muinonen, Karri; Granvik, Mikael; O'Mullane, William +7 more

We present two added-value interfaces (AVIs) for analyzing photometric and spectroscopic data observed by the Gaia satellite. The Gaia Added-Value Interface for Temporal Analysis (GAVITEA) is used to calculate an estimate for the spin state and shape of an asteroid from its photometric data, and the Gaia Added-Value Interface for Spectral Classifi…

2018 Advances in Space Research
Gaia 5
Collapse-driven formation of depressions on comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2017.11.019 Bibcode: 2018Icar..302..266L

Leliwa-Kopystynski, J.

The extremely diverse surface of comet 67P/Churyumov-Gerasimenko contains a large number of depressions or craters of very different scales. Among the most prominent are two large roughly circular depressions, each with radii of several hundred meters. In this work a model for the formation of the depressions is proposed. It is based on the theory…

2018 Icarus
Rosetta 5
SMHASH: a new mid-infrared RR Lyrae distance determination for the Local Group dwarf spheroidal galaxy Sculptor
DOI: 10.1093/mnras/sty2222 Bibcode: 2018MNRAS.481..578G

Majewski, Steven R.; Madore, Barry F.; Freedman, Wendy L. +12 more

We present a new distance estimation for the Milky Way dwarf spheroidal satellite Sculptor obtained from multi-epoch mid-infrared observations of RR Lyrae stars (RRLs). The 3.6 µm observations have been acquired with the Infrared Array Camera onboard the Spitzer Space Telescope as part of the SMHASH program. Mid-infrared light curves for 42 …

2018 Monthly Notices of the Royal Astronomical Society
Gaia 5
Probing the dynamical state, baryon content, and multiphase nature of galaxy clusters with bright background QSOs
DOI: 10.1093/mnras/sty2492 Bibcode: 2018MNRAS.481.4111G

Tripp, Todd M.; Burchett, Joseph N.; Wang, Q. Daniel +5 more

We have initiated a programme to study the physical/dynamical state of gas in galaxy clusters and the impact of the cluster environment on gaseous haloes of individual galaxies using X-ray imaging and UV absorption line spectroscopy of background QSOs. Here, we report results from the analysis Chandra and XMM-Newton archival data of five galaxy cl…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 5