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TYC 5353-1137-1: an enigmatic Doubly Periodic Variable of semiregular amplitude
DOI: 10.22444/IBVS.6248 Bibcode: 2018IBVS.6248....1R

Rosales, J. A., Mennickent, R. E.

2018 Information Bulletin on Variable Stars
Hipparcos 2
Global Maps of Energetic Ions in Saturn's Magnetosphere
DOI: 10.1029/2018JA025814 Bibcode: 2018JGRA..123.8557C

Mitchell, D. G.; Carbary, J. F.; Hamilton, D. C.

The Magnetospheric Imaging Instrument/Charge Energy Mass Spectrometer onboard the Cassini spacecraft measured suprathermal H+ and water group (W+) ions during the 13-year mission from 2004 to 2017. This paper generates statistical maps of pulse height analyzed fluxes for 3.24-3.34 keV H+ and 8.79-9.05 keV W+

2018 Journal of Geophysical Research (Space Physics)
Cassini 2
Modeling of Magnetic Dipolarizations and Turbulence in Earth's Magnetotail as Factors of Plasma Acceleration and Transfer
DOI: 10.1134/S0010952518060084 Bibcode: 2018CosRe..56..453P

Malova, H. V.; Popov, V. Yu.; Petrukovich, A. A. +4 more

2018 Cosmic Research
Cluster 2
Modelling the diffuse dust emission around Orion
DOI: 10.1093/mnras/sty578 Bibcode: 2018MNRAS.476.4690S

Shalima, P.; Gogoi, Rupjyoti; Saikia, Gautam

We have studied the diffuse radiation in the surroundings of M42 using photometric data from the Galaxy Evolution Explorer (GALEX) in the far-ultraviolet (FUV) and infrared observations of the AKARI space telescope. The main source of the FUV diffuse emission is the starlight from the Trapezium stars scattered by dust in front of the nebula. We in…

2018 Monthly Notices of the Royal Astronomical Society
AKARI IUE 2
Serendipitous X-Ray Sources in the Chandra HRC Field around Alpha Centauri
DOI: 10.3847/1538-3881/aaea62 Bibcode: 2018AJ....156..274A

Ayres, Thomas R.

For more than a decade, Alpha Centauri AB (G2 V+K1 V) has been observed by Chandra, in a long-term program to follow coronal (T ∼ 106 K) activity cycles of the two sunlike stars. Over 2008.4-2017.8, 19 HRC-I exposures were taken, each about 10 ks in duration, and spaced about six months apart. Beyond monitoring the AB X-ray luminosities…

2018 The Astronomical Journal
Gaia 2
KIC 2568888: To Be or Not to Be a Binary
DOI: 10.3847/1538-4357/aae846 Bibcode: 2018ApJ...868..103T

García, R. A.; De Ridder, J.; Mints, A. +4 more

In cases where both components of a binary system show oscillations, asteroseismology has been proposed as a method to identify the system. For KIC 2568888, observed with Kepler, we detect oscillation modes for two red giants in a single power-density spectrum. Through an asteroseismic study we investigate if the stars have similar properties, whi…

2018 The Astrophysical Journal
Gaia 2
Multiwavelength approach to classifying transient events in the direction of M 31
DOI: 10.1051/0004-6361/201732068 Bibcode: 2018A&A...615A.152S

Kong, Albert K. H.; Kupfer, Thomas; Laher, Russ R. +4 more

Context. In the hunt for rare time-domain events, it is important to consider confusing exotic extragalactic phenomena with more common Galactic foreground events.
Aims: We show how observations from multiple wavebands, in this case optical and X-ray observations, can be used to facilitate the distinction between the two.
Methods: We dis…

2018 Astronomy and Astrophysics
XMM-Newton 2
First Ten Years of Hinode Solar On-Orbit Observatory
DOI: 10.1007/978-981-10-7742-5 Bibcode: 2018ASSL..449.....S

Shimizu, Toshifumi; Kubo, Masahito; Imada, Shinsuke

2018 First Ten Years of Hinode Solar On-Orbit Observatory
Hinode 2
Solar Microflares Observed by SphinX and RHESSI
DOI: 10.1007/s11207-018-1319-0 Bibcode: 2018SoPh..293..101M

Mrozek, Tomasz; Kepa, Anna; Sylwester, Barbara +4 more

In 2009, the Russian Complex Orbital Observations Near-Earth of Activity of the Sun (CORONAS-Photon) spacecraft was launched, carrying the Polish Solar PHotometer In X-rays (SphinX). The SphinX was most sensitive in the spectral range 1.2 - 15 keV, thus an excellent opportunity appeared for comparison with the low-energy end of Ramaty High Energy …

2018 Solar Physics
Hinode 2
The Dust-selected Molecular Clouds in the Northeast Region of the Small Magellanic Cloud
DOI: 10.3847/1538-4357/aae48b Bibcode: 2018ApJ...867..117T

Kohno, Kotaro; Bot, Caroline; Yun, Min S. +19 more

We present a high-sensitivity (1σ < 1.6 mJy beam-1) continuum observation in a 343 arcmin2 area of the northeast region of the Small Magellanic Cloud at a wavelength of 1.1 mm, conducted using the AzTEC instrument on the ASTE telescope. In the observed region, we identified 20 objects by contouring 10σ emission. Through sp…

2018 The Astrophysical Journal
Herschel 2