Search Publications

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
WASP-92, WASP-93, and WASP-118: transit timing variations and long-term stability of the systems
DOI: 10.1093/mnras/stz676 Bibcode: 2019MNRAS.485.3580G

Evans, Phil; Gajdoš, Pavol; Vaňko, Martin +8 more

We studied three exoplanetary systems with transiting planets: WASP-92, WASP-93, and WASP-118. Using ground-based photometric observations of WASP-92 and WASP-93 and Kepler-K2 observations of WASP-118, we redetermined the orbital and physical parameters of these planets. The precise times of all transits were determined. We constructed O-C diagram…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 6
3D hydrodynamical models of point-symmetric planetary nebulae: the special case of H 1-67
DOI: 10.1093/mnras/sty2758 Bibcode: 2019MNRAS.482.1163R

Velázquez, P. F.; Peña, M.; Rechy-García, J. S.

We present 3D hydrodynamical simulations of a precessing jet with a time-dependent ejection velocity or a time-dependent ejection density, interacting with a circumstellar medium given by a dense, anisotropic, and slow AGB wind, forming a torus. We explore a set of configurations with different values for the precession angle and number of ejectio…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 6
Primeval very low-mass stars and brown dwarfs - V. A halo L3 subdwarf with prograde eccentric orbit in the Galactic plane
DOI: 10.1093/mnras/stz659 Bibcode: 2019MNRAS.486.1840Z

Burgasser, A. J.; Zhang, Z. H.; Smith, L. C.

VVV J12564163-6202039 is an L subdwarf located in the Galactic plane (b = 0{^{circ}.}831) discovered by its high proper motion (1.1 arcsec yr-1). We obtained an optical to near-infrared spectrum of it with the X-shooter on the Very Large Telescope, and re-classified it as an sdL3 subdwarf. Its best-fitting BT-Dusty model spec…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 6