Search Publications

A fractal analysis application of the pre-whitening technique to δ Scuti stars time series
DOI: 10.1093/mnras/stz1571 Bibcode: 2019MNRAS.487.4457D

Garrido, R.; Suárez, J. C.; de Franciscis, S. +4 more

Fractal fingerprints have been found recently in the light curves of several δ Scuti stars observed by Convection Rotation and planetary Transits(CoRoT) satellite. This sole fact might pose a problem for the detection of pulsation frequencies using classical pre-whitening techniques, but it is also a potentially rich source for information about p…

2019 Monthly Notices of the Royal Astronomical Society
CoRoT 7
Young stars raining through the galactic halo: the nature and orbit of price-whelan 1
DOI: 10.1093/mnras/stz2788 Bibcode: 2019MNRAS.490.2588B

Martin, Nicolas; Malhan, Khyati; Ibata, Rodrigo A. +3 more

We present radial velocities for five member stars of the recently discovered young (age ≃ 100-150 Myr) stellar system Price-Whelan 1 (PW 1), which is located far away in the Galactic Halo (D≃ 29 kpc, Z≃ 15 kpc), and that is probably associated with the leading arm (LA) of the Magellanic Stream. We measure the systemic radial velocity of PW 1, V

2019 Monthly Notices of the Royal Astronomical Society
Gaia 7
A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z ∼ 0.4
DOI: 10.1093/mnras/stz427 Bibcode: 2019MNRAS.485.1528A

Sánchez-Portal, Miguel; Pintos-Castro, Irene; Bongiovanni, Ángel +9 more

The well-known cluster of galaxies ZwCl0024+1652 at z ∼ 0.4 lacks an in-depth morphological classification of its central region. While previous studies provide a visual classification of a patched area, we used the public code called galaxy Support Vector Machine (GALSVM) and HST/ACS data as well as the WFP2 master catalogue to automatically clas…

2019 Monthly Notices of the Royal Astronomical Society
eHST 7
Properties of jet and surrounding material of GW/GRB 170817A
DOI: 10.1093/mnras/stz2735 Bibcode: 2019MNRAS.490.2822Z

Ziaeepour, Houri

We use published data in radio, optical, and X-ray bands to analyse and model afterglows of GW/GRB 170817A. Our analysis is based on a phenomenological gamma-ray burst generator model, which we previously used to study the prompt gamma-ray emission of this important transient. We find a multicomponent model and a few of its variants that are consi…

2019 Monthly Notices of the Royal Astronomical Society
eHST 7
XRB continuum fitting with sensitive high-energy X-ray detectors
DOI: 10.1093/mnras/stz045 Bibcode: 2019MNRAS.484.1202P

Fabian, A. C.; Tomsick, J. A.; Buisson, D. J. K. +4 more

The launch of the Nuclear Spectroscopic Telescope Array (NuSTAR) heralded a new era of sensitive high-energy X-ray spectroscopy for X-ray binaries (XRBs). In this paper we show how multiple physical parameters can be measured from the accretion disc spectrum when the high-energy side of the disc spectrum can be measured precisely using NuSTAR. Thi…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
GK Car and GZ Nor: two low-luminous, depleted RV Tauri stars
DOI: 10.1093/mnras/stz1967 Bibcode: 2019MNRAS.488.4033G

Gezer, I.; Van Winckel, H.; Kamath, D. +1 more

We performed a photometric and spectroscopic analysis of two RV Tauri stars: GK Car and GZ Nor. Both objects are surrounded by hot circumstellar dust. Their pulsation periods, derived from ASAS (All Sky Automated Survey) photometric time-series, have been used to derive their luminosities and distances via the period-luminosity-distance (PLC) rela…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 7
Candidates for non-pulsating stars located in the Cepheid instability strip in the Large Magellanic Cloud based on Strömgren photometry
DOI: 10.1093/mnras/stz2112 Bibcode: 2019MNRAS.489.3285N

Soszyński, I.; Smolec, R.; Udalski, A. +14 more

We present candidates for non-pulsating stars lying in the classical Cepheid instability strip based on the Optical Gravitational Lensing Experiment (OGLE) photometric maps combined with Strömgren photometry obtained with the 4.1-m Southern Astrophysical Research (SOAR) telescope, and Gaia Data Release 2 data in four fields in the Large Magellanic…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 7
Outflowing gas in a compact ionization cone in the Seyfert 2 galaxy ESO 153-G20
DOI: 10.1093/mnras/stz2333 Bibcode: 2019MNRAS.489.4111S

Robinson, Andrew; Fischer, Travis C.; Schnorr-Müller, Allan +14 more

We present two-dimensional ionized gas and stellar kinematics in the inner 1.4 × 1.9 kpc2 of the Seyfert 2 galaxy ESO 153-G20 obtained with the Gemini-South/Gemini multi-object spectrograph integral field unit (GMOS-IFU) at a spatial resolution of 250 pc and spectral resolution of 36 km s-1. Strong [O III], Hα, [N II] and [S …

2019 Monthly Notices of the Royal Astronomical Society
eHST 7
Dust evolution in the circumstellar disc of the unclassified B[e] star HD 50138
DOI: 10.1093/mnras/stz486 Bibcode: 2019MNRAS.485.3112V

Ábrahám, P.; Chen, L.; Varga, J. +3 more

We studied the disc of the unclassified B[e] star HD 50138 in order to explore its structure and to find indications for the evolutionary status of this system, whether it is a young Herbig Be or a post-main-sequence star. Using high spatial resolution interferometric measurements from MIDI instrument (N-band) on the Very Large Telescope Interfero…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 7
Molecular environs and triggered star formation around the large Galactic infrared bubble N 24
DOI: 10.1093/mnras/stz1269 Bibcode: 2019MNRAS.487.1517L

Li, Dalei; Tang, Xindi; Zhou, Jianjun +10 more

A multi-wavelength analysis of the large Galactic infrared bubble N 24 is presented in this paper in order to investigate the molecular and star-formation environment around expanding H II regions. Using archival data from Herschel and ATLASGAL, the distribution and physical properties of the dust over the entire bubble are studied. Using the Clum…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 7