Search Publications

X-ray analysis of the accreting supermassive black hole in the radio galaxy PKS 2251+11
DOI: 10.1051/0004-6361/201935176 Bibcode: 2019A&A...625A..26R

Tombesi, F.; Panessa, F.; Bruni, G. +2 more

Context. We have investigated the dichotomy between jetted and non-jetted active galactic nuclei (AGNs), focusing on the fundamental differences of these two classes in the accretion physics onto the central supermassive black hole (SMBH). We tested the validity of the unification model of AGNs through the characterization of the mutual interactio…

2019 Astronomy and Astrophysics
XMM-Newton 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
Reprint of "Evidence for color dichotomy in the primordial Neptunian Trojan population"
DOI: 10.1016/j.icarus.2019.113433 Bibcode: 2019Icar..334...79L

Smith, M.; D'Andrea, C. B.; Abbott, T. M. C. +45 more

In the current model of early Solar System evolution, the stable members of the Jovian and Neptunian Trojan populations were captured into resonance from the leftover reservoir of planetesimals during the outward migration of the giant planets. As a result, both Jovian and Neptunian Trojans share a common origin with the primordial disk population…

2019 Icarus
Gaia 3
A Recipe for Finding Stellar Radii, Temperatures, Surface Gravities, Metallicities, and Masses Using Spectral Lines
DOI: 10.3847/1538-4357/ab2fce Bibcode: 2019ApJ...882..148G

Gray, David F.; Kaur, Taranpreet

A recipe based on physical principles employs the observed equivalent widths of 10 spectral lines to model the photosphere of a target star. Coupled with the visual magnitude and an absolute flux calibration, the recipe yields the angular radius, effective temperature, surface gravity, and metallicity. With the addition of a parallax, a linear rad…

2019 The Astrophysical Journal
Gaia 3
Optical Spectrum of Distant OH/IR Star V1648 Aql (IRAS 19386+0155)
DOI: 10.1134/S1990341319030040 Bibcode: 2019AstBu..74..277K

Klochkova, V. G.; Tavolzhanskaya, N. S.

We present an optical spectrum of the star V1648 Aql (IRAS19386+0155) obtained at the 6-m SAO RAS telescope with a spectral resolution of R ≥ 60 000. Heliocentric radial velocity was measured from numerous metal absorptions is Vr = 10.18 ± 0.05 km s-1 (VLSR = 18.1 km s-1). We determined the atmospheric, …

2019 Astrophysical Bulletin
Gaia 3
ALMA, ATCA, and Spitzer Observations of the Luminous Extragalactic Supernova SN 1978K
DOI: 10.3847/1538-4357/aaf1a3 Bibcode: 2019ApJ...870...59S

Kotak, R.; Ryder, S. D.; Smith, I. A. +2 more

Only three extragalactic supernovae have been detected at late times at millimeter wavelengths: SN 1987A, SN 1978K, and SN 1996cr. SN 1978K is a remarkably luminous Type IIn supernova that remains bright at all wavelengths 40 years after its explosion. Here, we present Atacama Large Millimeter/submillimeter Array (ALMA) observations taken in 2016 …

2019 The Astrophysical Journal
AKARI 3
Kinetic Theory of Ion Acoustic Waves Observed at Comet 67P/Churyumov-Gerasimenko
DOI: 10.3847/2041-8213/ab2f8d Bibcode: 2019ApJ...880L..13R

Rehman, Saeed ur; Shah, Asif; Haque, Qamar ul

This work presents the resonance interaction of ion acoustic waves with the cometary plasma as observed at comet 67P/Churyumov-Gerasimenko. The plasma is comprised of cold, warm, and suprathermal electron populations and water ions such that the quasineutrality is satisfied. The cold electron population is found to play a dominant role in the damp…

2019 The Astrophysical Journal
Rosetta 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
Exploring the Asymmetry of the Solar Corona Electron Density with Very Long Baseline Interferometry
DOI: 10.3847/1538-4357/ab499a Bibcode: 2019ApJ...885..159A

Pavlov, Dmitry; Melnikov, Alexey; Aksim, Dan +1 more

The Sun’s corona has interested researchers for multiple reasons, including the search for a solution to the famous coronal heating problem and a purely practical consideration of predicting geomagnetic storms on Earth. There exist numerous different theories regarding the solar corona; therefore, it is important to be able to perform comparative …

2019 The Astrophysical Journal
SOHO Ulysses 3