Search Publications

Compact Galaxies at intermediate redshifts quench faster than normal-sized Galaxies
DOI: 10.1093/mnras/stz190 Bibcode: 2019MNRAS.484.3022N

Menéndez-Delmestre, K.; Charbonnier, A.; Gonçalves, T. S. +2 more

Massive quiescent compact galaxies have been discovered at high redshifts, associated with rapid compaction and cessation of star formation (SF). In this work, we set out to quantify the time-scales in which SF is quenched in compact galaxies at intermediate redshifts. For this, we select a sample of green valley galaxies within the COSMOS field i…

2019 Monthly Notices of the Royal Astronomical Society
eHST 8
Mode of accretion in episodic radio galaxies and the dynamics of their outer relic lobes
DOI: 10.1093/mnras/stz1089 Bibcode: 2019MNRAS.486.3975K

Hota, Ananda; Hardcastle, M. J.; Croston, J. H. +3 more

We present X-ray observations with the X-ray Multi-Mirror Mission Newton telescope of three double-double radio galaxies (DDRGs). We have detected the core, lobes, and environment of our sample DDRGs in X-rays. We examine the relationships between the radio and X-ray emission and attribute the X-ray emission from the lobes to the inverse Compton s…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 8
A new possible accretion scenario for ultra-luminous X-ray sources
DOI: 10.1093/mnras/stz2139 Bibcode: 2019MNRAS.489..366K

Makishima, K.; Nakazawa, K.; Kobayashi, Shogo B.

Using archival data from Suzaku, XMM-Newton, and NuSTAR, nine representative ultra-luminous X-ray sources (ULXs) in nearby galaxies were studied. Their X-ray spectra were all reproduced with a multicolour disc emission model plus its Comptonization. However, the spectral shapes of individual sources changed systematically depending on the luminosi…

2019 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 8
Evidence for bimodal orbital separations of white dwarf-red dwarf binary stars
DOI: 10.1093/mnras/stz298 Bibcode: 2019MNRAS.484.5362A

Gänsicke, B. T.; Marsh, T. R.; Ashley, R. P. +2 more

We present the results of a radial velocity survey of 20 white dwarf plus M dwarf binaries selected as a follow up to a Hubble Space Telescope study that aimed to spatially resolve suspected binaries. Our candidates are taken from the list of targets that were spatially unresolved with Hubble. We have determined the orbital periods for 16 of these…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 8
The GALANTE photometric system
DOI: 10.1093/mnras/stz842 Bibcode: 2019MNRAS.486..966L

Lennon, D. J.; García-Lario, P.; Maíz Apellániz, J. +9 more

This paper describes the characterization of the GALANTE photometric system, a seven intermediate- and narrow-band filter system with a wavelength coverage from 3000 Å to 9000 Å. We describe the photometric system presenting the full sensitivity curve as a product of the filter sensitivity, CCD, telescope mirror, and atmospheric transmission curve…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 8
Swift UVOT observations of the 2015 outburst of V404 Cygni
DOI: 10.1093/mnras/stz1998 Bibcode: 2019MNRAS.488.4843O

Altamirano, D.; Knigge, C.; Page, M. J. +10 more

The black hole binary, V404 Cygni, went into outburst in 2015 June, after 26 years of X-ray quiescence. We observed the outburst with the Neil Gehrels Swift observatory. We present optical/UV observations taken with the Swift Ultra-violet Optical Telescope, and compare them with the X-ray observations obtained with the Swift X-ray Telescope. We fi…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 8
Early-type galaxies in low-density environments: NGC 6876 explored through its globular cluster system
DOI: 10.1093/mnras/stz1660 Bibcode: 2019MNRAS.488..770E

Bassino, Lilia P.; Caso, Juan P.; Ennis, Ana I. +1 more

We present the results of a photometric study of the early-type galaxy NGC 6876 and the surrounding globular cluster (GC) system. The host galaxy is a massive elliptical, the brightest of this type in the Pavo Group. According to its intrinsic brightness (Mv ∼ -22.7), it is expected to belong to a galaxy cluster instead of a poor group.…

2019 Monthly Notices of the Royal Astronomical Society
eHST 8
Galactic resonance rings: modelling of motions in the wide solar neighbourhood
DOI: 10.1093/mnras/stz425 Bibcode: 2019MNRAS.485.2106M

Melnik, A. M.

Models of the Galaxy with analytical Ferrers bars can reproduce the residual velocities of OB associations in the Sagittarius, Perseus and Local System star-gas complexes located within 3 kpc of the solar neighbourhood. Ferrers ellipsoids with a density distribution defined by power indices n = 1 and 2 are considered. The successful reproduction o…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 8
A supragalactic conundrum: the globular clusters colour pattern in Virgo galaxies
DOI: 10.1093/mnras/sty2746 Bibcode: 2019MNRAS.482..950F

Forte, Juan C.; Vega, E. Irene; Geisler, Douglas +8 more

The presence of systematic modulations in the colour distributions in composite samples of globular clusters (GCs) associated with galaxies in the Virgo and Fornax clusters has been reported in a previous work. In this paper, we focus on the 27 brightest galaxies in Virgo, and in particular on NGC 4486, the dominant system in terms of GC populatio…

2019 Monthly Notices of the Royal Astronomical Society
eHST 7
VVV-WIT-07: another Boyajian's star or a Mamajek's object?
DOI: 10.1093/mnras/sty3004 Bibcode: 2019MNRAS.482.5000S

Minniti, D.; Saito, R. K.; Baptista, R. +6 more

We report the discovery of VVV-WIT-07, a unique and intriguing variable source presenting a sequence of recurrent dips with a likely deep eclipse in 2012 July. The object was found serendipitously in the near-IR data obtained by the VISTA Variables in the Vía Láctea (VVV) ESO public survey. Our analysis is based on VVV variability, multicolour, an…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 7