Search Publications

The GALAH survey: velocity fluctuations in the Milky Way using Red Clump giants
DOI: 10.1093/mnras/sty2924 Bibcode: 2019MNRAS.482.4215K

Lewis, Geraint F.; Ting, Yuan-Sen; Wittenmyer, Robert A. +20 more

If the Galaxy is axisymmetric and in dynamical equilibrium, we expect negligible fluctuations in the residual line-of-sight velocity field. Recent results using the APOGEE survey find significant fluctuations in velocity for stars in the mid-plane (|z| <0.25 kpc) out to 5 kpc, suggesting that the dynamical influence of non-axisymmetric features…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 11
Rest-frame UV and optical emission line diagnostics of ionized gas properties: a test case in a star-forming knot of a lensed galaxy at z ∼ 1.7
DOI: 10.1093/mnras/stz1987 Bibcode: 2019MNRAS.488.5862A

Kewley, Lisa J.; Blanc, Guillermo A.; Acharyya, Ayan +7 more

We examine the diagnostic power of rest-frame ultraviolet (UV) nebular emission lines, and compare them to more commonly used rest-frame optical emission lines, using the test case of a single star-forming knot of the bright lensed galaxy RCSGA 032727-132609 at redshift z ∼ 1.7. This galaxy has complete coverage of all the major rest-frame UV and …

2019 Monthly Notices of the Royal Astronomical Society
eHST 11
A newly discovered double-double candidate microquasar in NGC 300
DOI: 10.1093/mnras/sty2771 Bibcode: 2019MNRAS.482.2389U

Maccarone, T. J.; Motch, C.; Scaringi, S. +7 more

We present the discovery of a powerful candidate microquasar in NGC 300, associated with the S 10 optical nebula (previously classified as a supernova remnant). Chandra images show four discrete X-ray knots aligned in the plane of the sky over a length of ≈150 pc. The X-ray emission from the knots is well fitted with a thermal plasma model at a te…

2019 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton eHST 11
A short and sudden increase of the magnetic field strength and the accompanying spectral variability in the O9.7 V star HD 54879
DOI: 10.1093/mnras/stz198 Bibcode: 2019MNRAS.484.4495H

Hubrig, S.; Schöller, M.; Järvinen, S. P. +4 more

Only 11 O-type stars have been confirmed to possess large-scale organized magnetic fields. The presence of a -600 G longitudinal magnetic field in the O9.7 V star HD 54879 with a lower limit of the dipole strength of ∼2 kG was discovered a few years ago in the framework of the ESO large program `B-fields in OB stars'. Our FORS 2 spectropolarimetri…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 11
A remarkable change of the spectrum of the magnetic Of?p star HD 148937 reveals evidence of an eccentric, high-mass binary
DOI: 10.1093/mnras/sty3304 Bibcode: 2019MNRAS.483.2581W

Howarth, I. D.; Wade, G. A.; Gamen, R. +10 more

We report new spectroscopic observations of the magnetic Of?p star HD 148937 obtained since 2015 that differ qualitatively from its extensive historical record of weak, periodic spectral variations. This remarkable behaviour represents clear evidence for an unprecedented change in the character of variability of the star. In this paper, we describ…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 11
Identifications of faint Chandra sources in the globular cluster M3
DOI: 10.1093/mnras/sty3384 Bibcode: 2019MNRAS.483.4560Z

Heinke, Craig O.; Cool, Adrienne M.; Zhao, Yue +2 more

We report a 30 ksChandra ACIS-S survey of the globular cluster M3. Sixteen X-ray sources were detected within the half-light radius (2.3 arcmin) with L_X ≳ 2.3 × 10^{31} erg s^{-1}. We used Hubble Space Telescope WFC3/UVIS and ACS/WFC images to find 10 plausible optical/UV counterparts. We fit the spectral energy distribution of the known cataclys…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 10
PoGO+ polarimetric constraint on the synchrotron jet emission of Cygnus X-1
DOI: 10.1093/mnrasl/sly233 Bibcode: 2019MNRAS.483L.138C

Takahashi, Hiromitsu; Uchida, Nagomi; Kataoka, Jun +8 more

We report a polarimetric constraint on the hard X-ray synchrotron jet emission from the Cygnus X-1 black hole binary system. The observational data were obtained using the PoGO+ hard X-ray polarimeter in 2016 July, when Cygnus X-1 was in the hard state. We have previously reported that emission from an extended corona with a low polarization fract…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 10
The retrograde orbit of the globular cluster FSR1758 revealed with Gaia DR2
DOI: 10.1093/mnras/stz1699 Bibcode: 2019MNRAS.488..253S

Simpson, Jeffrey D.

We report the first radial velocity measurements of the recently identified globular cluster FSR1758. From the two member stars with radial velocities from the Gaia Radial Velocity Spectrograph reported in Gaia DR2, we find FSR1758 has a radial velocity of 227 ± 1 km s^{-1}. We also find potential extra-tidal star lost from the cluster in the surr…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 10
The relativistic jet of the γ-ray emitting narrow-line Seyfert 1 galaxy PKS J1222+0413
DOI: 10.1093/mnras/stz1193 Bibcode: 2019MNRAS.487..181K

Done, Chris; Angelakis, Emmanouil; Landt, Hermine +6 more

We present a multifrequency study of PKS J1222+0413 (4C +04.42), currently the highest redshift γ-ray emitting narrow-line Seyfert 1 (γ-NLS1). We assemble a broad spectral energy distribution (SED) including previously unpublished datasets: X-ray data obtained with the NuSTAR and Neil Gehrels Swift observatories; near-infrared, optical, and UV spe…

2019 Monthly Notices of the Royal Astronomical Society
Herschel XMM-Newton 10
The mid-infrared and CO gas properties of an extreme star-forming FeLoBAL quasar
DOI: 10.1093/mnras/stz1471 Bibcode: 2019MNRAS.487.3130P

Lacy, Mark; Hatziminaoglou, Evanthia; Afonso, José +6 more

We present a detailed study of a high-redshift iron low-ionization broad absorption line (FeLoBAL) quasar (SDSS1214 at z = 1.046), including new interferometric 12CO J = 2-1 observations, optical through far-infrared photometry, and mid-infrared spectroscopy. The CO line is well fit by a single Gaussian centred 40 km s-1 away…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 10