Search Publications

The M dwarf problem: Fe and Ti abundances in a volume-limited sample of M dwarf stars
DOI: 10.1093/mnras/staa878 Bibcode: 2020MNRAS.494.2718W

Wallerstein, George; Woolf, Vincent M.

We report iron and titanium abundance measurements from high-resolution spectra in a volume-limited sample of 106 M0 and M0.5 dwarf stars. The sample includes stars north of the celestial equator and closer than 29 parsecs. The results imply that there is an M dwarf problem similar to the previously known G dwarf problem, in that the fraction of l…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 9
Deviations from the Infrared-radio Correlation in Massive, Ultracompact Starburst Galaxies
DOI: 10.3847/1538-4357/abb19d Bibcode: 2020ApJ...901..138P

Moustakas, John; Coil, Alison L.; Rudnick, Gregory H. +11 more

Feedback through energetic outflows has emerged as a key physical process responsible for transforming star-forming galaxies into the quiescent systems observed in the local universe. To explore this process, this paper focuses on a sample of massive and compact merger remnant galaxies hosting high-velocity gaseous outflows ( $| v| \gtrsim {10}^{3…

2020 The Astrophysical Journal
eHST 9
A multiwavelength search for black widow and redback counterparts of candidate γ-ray millisecond pulsars
DOI: 10.1093/mnras/staa2339 Bibcode: 2020MNRAS.497.5364B

Tiengo, A.; Belfiore, A.; Marelli, M. +6 more

The wealth of detections of millisecond pulsars (MSPs) in γ-rays by Fermi has spurred searches for these objects among the several unidentified γ-ray sources. Interesting targets are a sub-class of binary MSPs, dubbed 'black widows' (BWs) and 'redbacks' (RBs), which are in orbit with low-mass non-degenerate companions fully or partially ablated by…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 9
Speckle Interferometry of Nearby Multiple Stars: 2007-2019 Positional Measurements and Orbits of Eight Objects
DOI: 10.3847/1538-3881/ab8ae2 Bibcode: 2020AJ....159..266M

Dyachenko, V.; Beskakotov, A.; Maksimov, A. +4 more

The orbits of eight systems with low-mass components (HIP 14524, HIP 16025, HIP 28671, HIP 46199, HIP 47791, HIP 60444, HIP 61100, and HIP 73085) are presented. Speckle interferometric data were obtained at the 6 m Big Telescope Alt-azimuth Special Astrophysical Observatory of the Russian Academy of Sciences (BTA SAO RAS) from 2007 to 2019. New da…

2020 The Astronomical Journal
Gaia Hipparcos 9
INTEGRAL results on the electron-positron annihilation radiation and X-ray & Gamma-ray diffuse emission of the Milky Way
DOI: 10.1016/j.newar.2020.101548 Bibcode: 2020NewAR..9001548C

Churazov, Eugene; Sunyaev, Rashid; Knödlseder, Jürgen +8 more

This review summarizes INTEGRAL results on two topics: the electron-positron annihilation line and X-ray & Gamma-ray diffuse emission of the Milky Way.

The electron-positron annihilation line at 511 keV is the most prominent spectral feature in the gamma-ray spectrum of the Milky Way. From the observational perspective, INTEGRAL has alrea…

2020 New Astronomy Reviews
INTEGRAL 9
ROBO-AO Kepler Asteroseismic Survey. II. Do Stellar Companions Inhibit Stellar Oscillations?
DOI: 10.3847/1538-4357/ab50c3 Bibcode: 2020ApJ...888...34S

Kulkarni, S. R.; Baranec, Christoph; Duev, Dmitry A. +7 more

The Kepler Space Telescope observed over 15,000 stars for asteroseismic studies. Of these, 75% of dwarfs (and 8% of giants) were found to show anomalous behavior, such as suppressed oscillations (low amplitude) or no oscillations at all. The lack of solar-like oscillations may be a consequence of multiplicity, due to physical interactions with spe…

2020 The Astrophysical Journal
Gaia 9
Keck Cosmic Web Imager (KCWI) spectra of globular clusters and ultracompact dwarfs in the halo of M87
DOI: 10.1093/mnras/staa1924 Bibcode: 2020MNRAS.497..765F

Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean P. +2 more

Using the Keck Cosmic Web Imager, we obtain spectra of several globular clusters (GCs), ultracompact dwarfs (UCDs), and the inner halo starlight of M87, at a similar projected galactocentric radius of ~5 kpc. This enables us, for the first time, to apply the same stellar population analysis to the GCs, UCDs, and starlight consistently to derive ag…

2020 Monthly Notices of the Royal Astronomical Society
eHST 9
Infrared properties of planetary nebulae with [WR] and wels central stars
DOI: 10.1093/mnras/staa217 Bibcode: 2020MNRAS.493..730M

Parthasarathy, M.; Muthumariappan, C.

We report the infrared (IR) properties of planetary nebulae (PNe) with Wolf-Rayet (WR) type and wels central stars known to date and compare them with the IR properties of a sample of PNe with H-rich central stars. We use near-, mid-, and far-IR photometric data from archives to derive the IR properties of PNe. We have constructed IR colour-colour…

2020 Monthly Notices of the Royal Astronomical Society
AKARI ISO 9
Hot gaseous atmospheres of rotating galaxies observed with XMM-Newton
DOI: 10.1093/mnras/staa3182 Bibcode: 2020MNRAS.499.5163J

Gaspari, M.; Nulsen, P. E. J.; Donahue, M. +6 more

X-ray emitting atmospheres of non-rotating early-type galaxies and their connection to central active galactic nuclei have been thoroughly studied over the years. However, in systems with significant angular momentum, processes of heating and cooling are likely to proceed differently. We present an analysis of the hot atmospheres of six lenticular…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 9
Ground-based visible spectroscopy of asteroids to support the development of an unsupervised Gaia asteroid taxonomy
DOI: 10.1051/0004-6361/202038246 Bibcode: 2020A&A...642A..80C

Tanga, P.; Galluccio, L.; Cellino, A. +4 more

Context. The Gaia mission of the European Space Agency is measuring reflectance spectra of a number to the order of 105 small Solar System objects. A first sample will be published in the Gaia Data Release scheduled for 2021.
Aims: The aim of our work was to test the procedure developed to obtain taxonomic classifications for aster…

2020 Astronomy and Astrophysics
Gaia 9