Search Publications

A large amount of diffuse molecular gases in the bar of the strongly barred galaxy NGC 1300: cause of the low star formation efficiency
DOI: 10.1093/mnras/staa1296 Bibcode: 2020MNRAS.495.3840M

Ohta, Kouji; Maeda, Fumiya; Fujimoto, Yusuke +2 more

In many barred galaxies, star formation efficiency (SFE) in the bar is lower than those in the arm and bar-end, and its cause has still not been clear. Focusing on the strongly barred galaxy NGC 1300, we investigate the possibility that the presence of a large amount of diffuse molecular gas, which would not contribute to the SF, makes the SFE low…

2020 Monthly Notices of the Royal Astronomical Society
eHST 26
The disintegrating old open cluster Czernik 3
DOI: 10.1093/mnras/staa2412 Bibcode: 2020MNRAS.498.2309S

Pandey, S. B.; Ojha, D. K.; Ghosh, S. K. +6 more

We have performed a detailed analysis of the Czernik 3 (Cz3) open cluster by using deep near-infrared photometry taken with TIRCAM2 on the 3.6 m Devasthal optical telescope along with the recently available high-quality proper motion data from the Gaia DR2 and deep photometric data from Pan-STARRS1. The cluster has a highly elongated morphology wi…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 26
Know thy star, know thy planet: chemo-kinematically characterizing TESS targets
DOI: 10.1093/mnras/stz3255 Bibcode: 2020MNRAS.491.4365C

Vanderburg, Andrew; Hawkins, Keith; Bowler, Brendan P. +2 more

The Transiting Exoplanet Survey Satellite (TESS) has already begun to discover what will ultimately be thousands of exoplanets around nearby cool bright stars. These potential host stars must be well understood to accurately characterize exoplanets at the individual and population levels. We present a catalogue of the chemo-kinematic properties of…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 26
Multi-timescale reverberation mapping of Mrk 335
DOI: 10.1093/mnras/staa2735 Bibcode: 2020MNRAS.498.4971M

Ingram, Adam; Mastroserio, Guglielmo; van der Klis, Michiel

Time lags due to X-ray reverberation have been detected in several Seyfert galaxies. The different traveltime between reflected and directly observed rays naturally causes this type of lag, which depends directly on the light-crossing time-scale of the system and hence scales with the mass of the central black hole. Featureless 'hard lags' not ass…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
Magnetic activity based on LAMOST medium-resolution spectra and the Kepler survey
DOI: 10.1093/mnras/staa942 Bibcode: 2020MNRAS.495.1252Z

Shi, Jianrong; Gao, Qi; Han, Xianming L. +6 more

Stellar magnetic activity is an interesting phenomenon in late-type stars. We use the medium-resolution spectroscopic observations of 406 069 late-type stars from LAMOST to explore their properties. We perform a statistical analysis on the magnetic activity of the stars and their associated physical parameters. Our samples are cross-matched with o…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 26
The dependence of Type Ia Supernovae SALT2 light-curve parameters on host galaxy morphology
DOI: 10.1093/mnras/staa3173 Bibcode: 2020MNRAS.499.5121P

Pruzhinskaya, M. V.; Pauna, N.; Novinskaya, A. K. +1 more

Type Ia Supernovae (SNe Ia) are widely used to measure distances in the Universe. Despite the recent progress achieved in SN Ia standardization, the Hubble diagram still shows some remaining intrinsic dispersion. The remaining scatter in supernova luminosity could be due to the environmental effects that are accounted for as mass step correction i…

2020 Monthly Notices of the Royal Astronomical Society
eHST 26
Unlocking Galactic Wolf-Rayet stars with Gaia DR2 - II. Cluster and association membership
DOI: 10.1093/mnras/staa1290 Bibcode: 2020MNRAS.495.1209R

Parker, Richard J.; Crowther, Paul A.; Rate, Gemma

Galactic Wolf-Rayet (WR) star membership of star-forming regions can be used to constrain the formation environments of massive stars. Here, we utilize Gaia DR2 parallaxes and proper motions to reconsider WR star membership of clusters and associations in the Galactic disc, supplemented by recent near-infrared studies of young massive clusters. We…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 26
The Cluster AgeS Experiment (CASE) - VIII. Age and distance of the Globular Cluster 47 Tuc from the analysis of two detached eclipsing binaries
DOI: 10.1093/mnras/staa032 Bibcode: 2020MNRAS.492.4254T

Soszyński, I.; Udalski, A.; Szymański, M. K. +20 more

We use photometric and spectroscopic observations of the eclipsing binary E32 in the globular cluster 47 Tuc to derive the masses, radii, and luminosities of the component stars. The system has an orbital period of 40.9 d, a markedly eccentric orbit with e = 0.24, and is shown to be a member of or a recent escaper from the cluster. We obtain M_p =…

2020 Monthly Notices of the Royal Astronomical Society
Gaia eHST 26
The first broad-band X-ray view of the narrow-line Seyfert 1 Ton S180
DOI: 10.1093/mnras/staa2076 Bibcode: 2020MNRAS.497.2352M

Ebrero, J.; Schartel, N.; Santos-Lleó, M. +15 more

We present joint XMM-Newton and NuSTAR observations of the 'bare' narrow-line Seyfert 1 Ton S180 (z = 0.062), carried out in 2016 and providing the first hard X-ray view of this luminous galaxy. We find that the 0.4-30 keV band cannot be self-consistently reproduced by relativistic reflection models, which fail to account simultaneously for the so…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
A DECam view of the diffuse dwarf galaxy Crater II - Variable stars
DOI: 10.1093/mnras/stz3393 Bibcode: 2020MNRAS.492.1061V

Nidever, David L.; Olsen, Knut; Walker, Alistair R. +11 more

Time series observations of a single dithered field centred on the diffuse dwarf satellite galaxy Crater II were obtained with the Dark Energy Camera (DECam) at the 4m Blanco Telescope at Cerro Tololo Inter-American Observatory, Chile, uniformly covering up to two half-light radii. Analysis of the g and I time series results in the identification …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 26