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Characterization of the HD 219134 multiplanet system I. Observations of stellar magnetism, wind, and high-energy flux
DOI: 10.1093/mnras/sty2494 Bibcode: 2018MNRAS.481.5286F

Petit, P.; Vidotto, A. A.; Murthy, J. +9 more

HD 219134 hosts several planets, with seven candidates reported, and the two shortest period planets are rocky (4-5 M) and transit the star. Here, we present contemporaneous multiwavelength observations of the star HD 219134. We observed HD 219134 with the Narval spectropolarimeter at the Observatoire du Pic du Midi and used Zeeman-Dop…

2018 Monthly Notices of the Royal Astronomical Society
eHST 25
Disclosing the properties of low-redshift dual AGN through XMM-Newton and SDSS spectroscopy
DOI: 10.1093/mnras/sty1867 Bibcode: 2018MNRAS.480.1639D

Komossa, S.; Guainazzi, Matteo; Paragi, Zsolt +10 more

We report on an optical (SDSS) and X-ray (XMM-Newton) study of an optically selected sample of four dual AGN systems at projected separations of 30-60 kpc. All sources are detected in the X-ray band (0.3-10keV); seven objects are optically identified as Seyfert, while one source, optically classified as a low-ionization nuclear emission-line regio…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 25
A possible solution of the puzzling variation of the orbital period of MXB 1659-298
DOI: 10.1093/mnras/stx2529 Bibcode: 2018MNRAS.473.3490I

Sanna, A.; Di Salvo, T.; Burderi, L. +6 more

MXB 1659-298 is a transient neutron-star low-mass X-ray binary system that shows eclipses with a periodicity of 7.1 h. MXB 1659-298 went to outburst in 2015 August, after 14 years of quiescence. We investigate the orbital properties of this source with a baseline of 40 years, obtained by combining the eight eclipse arrival times present in the lit…

2018 Monthly Notices of the Royal Astronomical Society
XMM-Newton 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
ΛCDM predictions for the satellite population of M33
DOI: 10.1093/mnras/sty1946 Bibcode: 2018MNRAS.480.1883P

Carlin, Jeffrey L.; Patel, Ekta; Tollerud, Erik J. +2 more

Triangulum (M33) is the most massive satellite galaxy of Andromeda (M31), with a stellar mass of about 3 × 109 M. Based on abundance matching techniques, M33's total mass at infall is estimated to be of order 1011 M. ΛCDM simulations predict that M33-mass halos host several of their own low-mass satell…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 25
A 100 kpc nebula associated with the `Teacup' fading quasar
DOI: 10.1093/mnras/stx2911 Bibcode: 2018MNRAS.474.2302V

Humphrey, A.; Villar-Martín, M.; Ramos Almeida, C. +4 more

We report the discovery of an ∼100 kpc ionized nebula associated with the radio-quiet type 2 quasar (QSO2) nicknamed the `Teacup' (z = 0.085). The giant nebula is among the largest known around active galaxies at any z. We propose that it is part of the circumgalactic medium (CGM) of the QSO2 host, which has been populated with tidal debris by gal…

2018 Monthly Notices of the Royal Astronomical Society
eHST 25
NGTS-2b: an inflated hot-Jupiter transiting a bright F-dwarf
DOI: 10.1093/mnras/sty2581 Bibcode: 2018MNRAS.481.4960R

Smalley, Barry; Wheatley, Peter J.; Bayliss, Daniel +42 more

We report the discovery of NGTS-2b, an inflated hot-Jupiter transiting a bright F5V star (2MASS J14202949 - 3112074; Teff = 6478^{+94}_{-89} K), discovered as part of the Next Generation Transit Survey (NGTS). The planet is in a P = 4.51 d orbit with mass 0.74^{+0.13}_{-0.12}MJ, radius 1.595^{+0.047}_{-0.045}RJ, an…

2018 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 24
A refined search for pulsations in white dwarf companions to millisecond pulsars
DOI: 10.1093/mnras/sty1546 Bibcode: 2018MNRAS.479.1267K

Hermes, J. J.; Althaus, Leandro G.; Gianninas, A. +7 more

We present optical high-speed photometry of three millisecond pulsars with low-mass (<0.3 M) white dwarf companions, bringing the total number of such systems with follow-up time-series photometry to five. We confirm the detection of pulsations in one system, the white dwarf companion to PSR J1738+0333, and show that the pulsation f…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 24
The velocity ellipsoid in the Galactic disc using Gaia DR1
DOI: 10.1093/mnras/stx2774 Bibcode: 2018MNRAS.474..854A

Majewski, Steven R.; Anguiano, Borja; Freeman, Kenneth C. +2 more

The stellar velocity ellipsoid of the solar neighbour (d < 200 pc) is re-examined using intermediate-old mono-abundance stellar groups with high-quality chemistry data together with parallaxes and proper motions from Gaia DR1. We find the average velocity dispersion values for the three space velocity components for the thin and thick discs of …

2018 Monthly Notices of the Royal Astronomical Society
Gaia 24
Verifying reddening and extinction for Gaia DR1 TGAS giants
DOI: 10.1093/mnras/stx3251 Bibcode: 2018MNRAS.475.1121G

Gontcharov, George A.; Mosenkov, Aleksandr V.

Gaia DR1 Tycho-Gaia Astrometric Solution parallaxes, Tycho-2 photometry, and reddening/extinction estimates from nine data sources for 38 074 giants within 415 pc from the Sun are used to compare their position in the Hertzsprung-Russell diagram with theoretical estimates, which are based on the PARSEC and MIST isochrones and the TRILEGAL model of…

2018 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 24