Search Publications

Dust and gas emission from cometary nuclei: the case of comet 67P/Churyumov-Gerasimenko
DOI: 10.1080/23746149.2017.1404436 Bibcode: 2018AdPhX...304436K

Kramer, Tobias; Noack, Matthias; Baum, Daniel +2 more

2018 Advances in Physics X
Rosetta 11
NuSTAR rules out a cyclotron line in the accreting magnetar candidate 4U2206+54
DOI: 10.1093/mnras/sty1628 Bibcode: 2018MNRAS.479.3366T

Reig, P.; Torrejón, J. M.; Postnov, K. +3 more

Based on our new NuSTAR X-ray telescope data, we rule out any cyclotron line up to 60 keV in the spectra of the high-mass X-ray binary 4U2206+54. In particular, we do not find any evidence of the previously claimed line around 30 keV, independently of the source flux, along the spin pulse. The spin period has increased significantly, since the las…

2018 Monthly Notices of the Royal Astronomical Society
INTEGRAL 11
Exploring the spectral variability of the Seyfert 1.5 galaxy Markarian 530 with Suzaku
DOI: 10.1093/mnras/sty1306 Bibcode: 2018MNRAS.478.4214E

Gallo, L. C.; Gonzalez, A. G.; Ehler, H. J. S.

A 2012 Suzaku observation of the Seyfert 1.5 galaxy Markarian 530 was analysed and found to exhibit two distinct modes of variability, which were found to be independent from one another. First, the spectrum undergoes a smooth transition from a soft to hard spectrum. Secondly, the spectrum displays more rapid variability seemingly confined to a ve…

2018 Monthly Notices of the Royal Astronomical Society
Suzaku 11
Oxygen and silicon abundances in Cygnus OB2. Chemical homogeneity in a sample of OB slow rotators
DOI: 10.1051/0004-6361/201833989 Bibcode: 2018A&A...620A..56B

Herrero, A.; Comerón, F.; Simón-Díaz, S. +3 more

Context. Cygnus OB2 is a rich OB association in the Galaxy located at only ∼1.4 kpc from us which has experienced intense star formation in the last 20-25 Myr. Its stellar population shows a correlation between age and Galactic longitude. Exploring the chemical composition of its stellar content we will be able to check the degree of homogeneity o…

2018 Astronomy and Astrophysics
Gaia 11
Aerosol properties in the upper clouds of Venus from glory observations by the Venus Monitoring Camera (Venus Express mission)
DOI: 10.1016/j.icarus.2017.08.011 Bibcode: 2018Icar..299..272M

Markiewicz, Wojciech J.; Petrova, Elena V.; Shalygina, Oksana S.

From the angular positions of the glory features observed on the upper cloud deck of Venus in three VMC channels (at 0.365, 0.513, and 0.965 µm), the dominating sizes of cloud particles and their refractive indices have been retrieved, and their spatial and temporal variations have been analyzed. For this, the phase profiles of brightness we…

2018 Icarus
VenusExpress 11
Size-Luminosity Scaling Relations of Local and Distant Star-forming Regions
DOI: 10.3847/1538-4357/aaeb8f Bibcode: 2018ApJ...869...11C

Do, Tuan; Armus, Lee; Larkin, James E. +8 more

We investigate star-forming scaling relations using Bayesian inference on a comprehensive data sample of low- (z < 0.1) and high-redshift (1 < z < 5) star-forming regions. This full data set spans a wide range of host galaxy stellar mass (M * ∼ 106-1011 {M}) and clump star formation rates (SFR…

2018 The Astrophysical Journal
eHST 11
In-flight performance of pulse-processing system of the ASTRO-H/Hitomi soft x-ray spectrometer
DOI: 10.1117/1.JATIS.4.1.011217 Bibcode: 2018JATIS...4a1217I

Tsujimoto, Masahiro; Eckart, Megan E.; Leutenegger, Maurice A. +15 more

We summarize results of the initial in-orbit performance of the pulse shape processor (PSP) of the soft x-ray spectrometer instrument onboard ASTRO-H (Hitomi). Event formats, kind of telemetry, and the pulse-processing parameters are described, and the parameter settings in orbit are listed. The PSP was powered-on 2 days after launch, and the even…

2018 Journal of Astronomical Telescopes, Instruments, and Systems
Hitomi 11
Complete IRAC Mapping of the CFHTLS-DEEP, MUSYC, and NMBS-II Fields
DOI: 10.1088/1538-3873/aae796 Bibcode: 2018PASP..130l4501A

Muzzin, Adam; van Dokkum, Pieter; Bezanson, Rachel +19 more

The IRAC mapping of the NMBS-II fields program is an imaging survey at 3.6 and 4.5 µm with the Spitzer Infrared Array Camera (IRAC). The observations cover three Canada-France-Hawaii Telescope Legacy Survey Deep (CFHTLS-D) fields, including one also imaged by AEGIS, and two MUSYC fields. These are then combined with archival data from all pr…

2018 Publications of the Astronomical Society of the Pacific
eHST 11
On the Performance of Multi-Instrument Solar Flare Observations During Solar Cycle 24
DOI: 10.1007/s11207-017-1233-x Bibcode: 2018SoPh..293...18M

Milligan, Ryan O.; Ireland, Jack

The current fleet of space-based solar observatories offers us a wealth of opportunities to study solar flares over a range of wavelengths. Significant advances in our understanding of flare physics often come from coordinated observations between multiple instruments. Consequently, considerable efforts have been, and continue to be, made to coord…

2018 Solar Physics
Hinode IRIS PROBA-2 11
Extremely Low-Frequency Waves Inside the Diamagnetic Cavity of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1029/2017GL076415 Bibcode: 2018GeoRL..45.3854M

Gunell, H.; Eriksson, A.; Karlsson, T. +7 more

The European Space Agency/Rosetta mission to comet 67P/Churyumov-Gerasimenko has provided several hundred observations of the cometary diamagnetic cavity induced by the interaction between outgassed cometary particles, cometary ions, and the solar wind magnetic field. Here we present the first electric field measurements of four preperihelion and …

2018 Geophysical Research Letters
Rosetta 11