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Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar
DOI: 10.1126/sciadv.aao7228 Bibcode: 2018SciA....4.7228C

de Palma, Francesco; Fusco, Piergiorgio; Gargano, Fabio +129 more

Millisecond pulsars (MSPs) are old neutron stars that spin hundreds of times per second and appear to pulsate as their emission beams cross our line of sight. To date, radio pulsations have been detected from all rotation-powered MSPs. In an attempt to discover radio-quiet gamma-ray MSPs, we used the aggregated power from the computers of tens of …

2018 Science Advances
XMM-Newton 25
Wolf 1130: A Nearby Triple System Containing a Cool, Ultramassive White Dwarf
DOI: 10.3847/1538-4357/aaa8dd Bibcode: 2018ApJ...854..145M

Skiff, Brian A.; Kirkpatrick, J. Davy; Kim, Hwihyun +9 more

Following the discovery of the T8 subdwarf WISE J200520.38+542433.9 (Wolf 1130C), which has a proper motion in common with a binary (Wolf 1130AB) consisting of an M subdwarf and a white dwarf, we set out to learn more about the old binary in the system. We find that the A and B components of Wolf 1130 are tidally locked, which is revealed by the c…

2018 The Astrophysical Journal
Gaia eHST 25
XMM-Newton detection of the 2.1 ms coherent pulsations from IGR J17379-3747
DOI: 10.1051/0004-6361/201833205 Bibcode: 2018A&A...616L..17S

Sanna, A.; Ferrigno, C.; Papitto, A. +7 more

We report the detection of X-ray pulsations at 2.1 ms from the known X-ray burster IGR J17379-3747 using XMM-Newton. The coherent signal shows a clear Doppler modulation from which we estimate an orbital period of 1.9 h and a projected semi-major axis of 8 lt-ms. Taking into account the lack of eclipses (inclination angle of <75°) and assuming …

2018 Astronomy and Astrophysics
INTEGRAL XMM-Newton 25
A Spectral and Timing Study of MAXI J1535-571, Based on Swift/XRT, XMM-Newton, and NICER Observations Obtained in Fall 2017
DOI: 10.3847/1538-4357/aae7d3 Bibcode: 2018ApJ...868...71S

Stiele, H.; Kong, A. K. H.

We present a spectral-timing analysis of observations taken in fall 2017 of the newly detected X-ray transient MAXI J1535-571. We included 38 Swift/XRT window timing mode observations, 3 XMM-Newton observations, and 31 Neutron star Interior Composition Explorer observations in our study. We computed the fundamental diagrams commonly used to study …

2018 The Astrophysical Journal
XMM-Newton 25
The LatHyS database for planetary plasma environment investigations: Overview and a case study of data/model comparisons
DOI: 10.1016/j.pss.2017.02.015 Bibcode: 2018P&SS..150...13M

André, N.; Fedorov, A.; Budnik, E. +19 more

We present the Latmos Hybrid Simulation (LatHyS) database, which is dedicated to the investigations of planetary plasma environment. Simulation results of several planetary objects (Mars, Mercury, Ganymede) are available in an online catalogue. The full description of the simulations and their results is compliant with a data model developped in t…

2018 Planetary and Space Science
MEx 25
Probing the Southern Fermi Bubble in Ultraviolet Absorption Using Distant AGNs
DOI: 10.3847/1538-4357/aac167 Bibcode: 2018ApJ...860...98K

Jenkins, Edward B.; Jorgenson, Regina A.; Savage, Blair D. +7 more

The Fermi Bubbles are two giant gamma-ray emitting lobes extending 55° above and below the Galactic center. While the Northern Bubble has been extensively studied in ultraviolet (UV) absorption, little is known about the gas kinematics of the southern Bubble. We use UV absorption-line spectra from the Cosmic Origins Spectrograph (COS) on the Hubbl…

2018 The Astrophysical Journal
eHST 25
Physical properties and chemical composition of the cores in the California molecular cloud
DOI: 10.1051/0004-6361/201833622 Bibcode: 2018A&A...620A.163Z

Li, Di; Liu, Tie; Liu, Sheng-Yuan +13 more


Aims: We aim to reveal the physical properties and chemical composition of the cores in the California molecular cloud (CMC), so as to better understand the initial conditions of star formation.
Methods: We made a high-resolution column density map (18.2'') with Herschel data, and extracted a complete sample of the cores in the CMC with …

2018 Astronomy and Astrophysics
Herschel 25
A Comparative Study of WASP-67 b and HAT-P-38 b from WFC3 Data
DOI: 10.3847/1538-3881/aaa0c7 Bibcode: 2018AJ....155...55B

Deming, Drake; Stevenson, Kevin B.; Wakeford, Hannah R. +12 more

Atmospheric temperature and planetary gravity are thought to be the main parameters affecting cloud formation in giant exoplanet atmospheres. Recent attempts to understand cloud formation have explored wide regions of the equilibrium temperature-gravity parameter space. In this study, we instead compare the case of two giant planets with nearly id…

2018 The Astronomical Journal
eHST 25
Suppressed phase variations in a high amplitude rapidly oscillating Ap star pulsating in a distorted quadrupole mode
DOI: 10.1093/mnras/sty248 Bibcode: 2018MNRAS.476..601H

Saio, H.; Bowman, D. M.; Smalley, B. +5 more

We present the results of a multisite photometric observing campaign on the rapidly oscillating Ap (roAp) star 2MASS 16400299-0737293 (J1640; V = 12.7). We analyse photometric B data to show the star pulsates at a frequency of 151.93 d-1 (1758.45 µHz; P = 9.5 min) with a peak-to-peak amplitude of 20.68 mmag, making it one of the h…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 25
CMB constraints on β-exponential inflationary models
DOI: 10.1088/1475-7516/2018/03/023 Bibcode: 2018JCAP...03..023S

Alcaniz, J. S.; Silva, R.; Benetti, M. +2 more

We analyze a class of generalized inflationary models proposed in ref. [1], known as β-exponential inflation. We show that this kind of potential can arise in the context of brane cosmology, where the field describing the size of the extra-dimension is interpreted as the inflaton. We discuss the observational viability of this class of model in li…

2018 Journal of Cosmology and Astroparticle Physics
Planck 25