Search Publications

MHD simulation of the solar wind flow around the coma of comet Churyumov-Gerasimenko during Rosetta's flyby
DOI: 10.1093/mnras/sty3080 Bibcode: 2019MNRAS.482.5642B

Baranov, V. B.; Alexashov, D. B.; Lebedev, M. G.

The magnetohydrodynamic (MHD) model of the interaction between the solar wind and a cometary ionosphere is applied to investigate certain peculiar features of the solar wind flow around comet Churyumov-Gerasimenko during Rosetta's flyby at this comet. The model accounts for photoionization of the neutral component of the cometary outflow and the r…

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 3
A method to analyse velocity structure
DOI: 10.1093/mnras/sty3409 Bibcode: 2019MNRAS.483.3894A

Arnold, Becky; Goodwin, Simon P.

We present a new method of analysing and quantifying velocity structure in star-forming regions suitable for the rapidly increasing quantity and quality of stellar position-velocity data. The method can be applied to data in any number of dimensions, does not require the centre or characteristic size (e.g. radius) of the region to be determined, a…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 3
Early science with the Large Millimetre Telescope: new mm-wave detections of circumstellar discs in IC 348 from LMT/AzTEC
DOI: 10.1093/mnras/stz1739 Bibcode: 2019MNRAS.488.1462P

Gutermuth, Robert A.; Lane, James; Wilson, Grant W. +2 more

We present the most complete sample of mm measurements of protoplanetary discs in the star-forming region IC 348 to date. New observations from the Large Millimetre Telescope and the 1.1 mm camera AzTEC are combined with literature results in order to characterize the disc population as relating to both stellar properties within the IC 348 region …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 3
Results from the SuperModel analysis of the X-COP galaxy clusters sample
DOI: 10.1093/mnras/stz482 Bibcode: 2019MNRAS.485.1800F

Fusco-Femiano, Roberto

In this work, the analysis of the stacked projected temperature profile of 12 galaxy clusters of the X-COP sample is performed via the SuperModel, a tool for investigating the intracluster medium thermodynamic properties already tested on many clusters since 2009. Two separate fits have been carried out: to the joint X-ray and SZ-projected tempera…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 3
A catalogue of nuclear stellar velocity dispersions of nearby galaxies from Hα STIS spectra to constrain supermassive black hole masses
DOI: 10.1093/mnras/sty2918 Bibcode: 2019MNRAS.483...57P

Sarzi, Marc; Dalla Bontà, Elena; Corsini, Enrico Maria +4 more

We present new measurements for the nuclear stellar velocity dispersion σ* within sub-arcsecond apertures for 28 nearby galaxies. Our data consist of Space Telescope Imaging Spectrograph (STIS) long-slit spectra obtained with the G750M grating centred on the Hα spectral range. We fit the spectra using a library of single stellar populat…

2019 Monthly Notices of the Royal Astronomical Society
eHST 3
High-resolution spectroscopy of Boyajian's star during optical dimming events
DOI: 10.1093/mnras/stz850 Bibcode: 2019MNRAS.486..236M

Simón-Díaz, S.; Collier Cameron, A.; González Hernández, J. I. +13 more

Boyajian's star is an apparently normal main-sequence F-type star with a very unusual light curve. The dipping activity of the star, discovered during the Kepler mission, presents deep, asymmetric, and aperiodic events. Here we present high-resolution spectroscopic follow-up during some dimming events recorded post-Kepler observations, from ground…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 3
Parameter estimation for scarce stellar populations
DOI: 10.1093/mnras/stz1132 Bibcode: 2019MNRAS.486.5567R

Bitsakis, T.; Bruzual, G.; Cervantes Sodi, B. +1 more

We present a Bayesian method to determine simultaneously the age, metallicity, distance modulus, and interstellar reddening by dust of any resolved stellar population, by comparing the observed and synthetic colour magnitude diagrams on a star by star basis, with no need to bin the data into a carefully selected magnitude grid. We test the method …

2019 Monthly Notices of the Royal Astronomical Society
eHST 3
Absolute parameters of young stars: HX Velorum
DOI: 10.1093/mnras/stz1136 Bibcode: 2019MNRAS.487..161B

Demircan, O.; Özkardeş, B.; Erdem, A. +4 more

We present combined photometric and spectroscopic analyses of the southern multiple star HX Vel. High-resolution spectra of this system were taken at the University of Canterbury Mt. John Observatory in the years 2009-2015. Absolute parameters for HX Vel tend to confirm its young and near-main-sequence nature. We specify the main adopted parameter…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 3
A high signal-to-noise HST spectrum towards J1009+0713: precise absorption measurements in the CGM of two galaxies
DOI: 10.1093/mnras/stz2108 Bibcode: 2019MNRAS.489...78L

Nicastro, Fabrizio; Mathur, Smita; Weinberg, David H. +6 more

High signal-to-noise spectra towards background quasars are crucial for uncovering weak absorption in the circumgalactic medium (CGM) of intervening galaxies, such as the diagnostic lines of N V that provide insight to the ionization process of warm gas but typically have low equivalent widths. We present a new spectrum from the Hubble Space Teles…

2019 Monthly Notices of the Royal Astronomical Society
eHST 3
Differential astrometric framework for the Jupiter relativistic experiment with Gaia
DOI: 10.1093/mnras/stz452 Bibcode: 2019MNRAS.485.1147A

Abbas, Ummi; Bucciarelli, Beatrice; Lattanzi, Mario G.

We employ differential astrometric methods to establish a small field reference frame stable at the microarcsecond (µas) level on short time-scales using high-cadence simulated observations taken by Gaia in 2017 February of a bright star close to the limb of Jupiter, as part of the relativistic experiment on Jupiter's quadrupole. We achieve …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 3