Search Publications

Detection of Hα emission from PZ Telescopii B using SPHERE/ZIMPOL
DOI: 10.1051/0004-6361/201936510 Bibcode: 2019A&A...631A..84M

Henning, Thomas; Musso Barcucci, Arianna; Launhardt, Ralf +6 more

Hα is a powerful tracer of accretion and chromospheric activity, which has been detected in the case of young brown dwarfs and even recently in planetary mass companions (e.g. PDS70 b and c). Hα detections and characterisation of brown dwarf and planet companions can further our knowledge of their formation and evolution, and expanding such a samp…

2019 Astronomy and Astrophysics
Gaia 6
SN 2016B a.k.a. ASASSN-16ab: a transitional Type II supernova
DOI: 10.1093/mnras/stz949 Bibcode: 2019MNRAS.486.2850D

Pandey, S. B.; Benetti, S.; Kumar, Brajesh +12 more

We present photometry, polarimetry, and spectroscopy of the Type II supernova ASASSN-16ab/SN 2016B in PGC 037392. The photometric and spectroscopic follow-up commenced about 2 weeks after shock breakout and continued until nearly 6 months. The light curve of SN 2016B exhibits intermediate properties between those of Type IIP and IIL. The early dec…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 6
Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240)
DOI: 10.1051/0004-6361/201834159 Bibcode: 2019A&A...621A..25F

Rosado, M.; Amram, P.; Fuentes-Carrera, I. +6 more

Context. Encounters between galaxies modify their morphology, kinematics, and star formation history. The relation between these changes and external perturbations is not straightforward. The great number of parameters involved requires both the study of large samples and individual encounters where particular features, motions, and perturbations …

2019 Astronomy and Astrophysics
eHST 6
On ancient solar-type stars
DOI: 10.1093/mnras/sty2660 Bibcode: 2019MNRAS.482..471F

Fuhrmann, Klaus; Chini, Rolf

We describe a survey of ancient solar-type stars down to main-sequence effective temperatures Teff ≥ 5300 K and within 42 pc of the Sun. The underlying Gaia-based, volume-complete parent sample consists of 1633 sources, dominated by Population I. The design of the survey is such that around 130 sources are expected to be members of Popu…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 6
Acceleration of plasma in current sheet during substorm dipolarizations in the Earth's magnetotail: Comparison of different mechanisms
DOI: 10.1063/1.5082715 Bibcode: 2019PhPl...26d2901P

Parkhomenko, Elena I.; Malova, Helmi V.; Grigorenko, Elena E. +6 more

This work is devoted to the investigation of particle acceleration during magnetospheric dipolarizations. A numerical model is presented taking into account the four scenarios of plasma acceleration that can be realized: (A) total dipolarization with characteristic time scales of ≈3 min; (B) single peak value of the normal magnetic component

2019 Physics of Plasmas
Cluster 6
DS Andromedae: A Detached Eclipsing Double-lined Spectroscopic Binary in the Galactic Cluster NGC 752
DOI: 10.3847/1538-3881/ab22ba Bibcode: 2019AJ....158...82M

Frandsen, S.; Milone, E. F.; Schiller, S. J. +1 more

The Wilson-Devinney program has been used to analyze well-calibrated photometric and new radial velocity data to determine the properties and distance of DS Andromedae, a 1.01 day period, double-lined, totally eclipsing binary system of early-F spectral type and a likely member of the intermediate-age open cluster NGC 752. The determinations of ma…

2019 The Astronomical Journal
Gaia 6
On the Properties of the Galactic Dust Layer within 700 pc of the Sun
DOI: 10.1134/S1063773719080036 Bibcode: 2019AstL...45..605G

Gontcharov, G. A.

We compare the spatial stellar color variations with our three-dimensional analytical model of the spatial dust distribution to refine the properties of the dust layer in Galactic solar neighborhoods. We use a complete sample of 93 992 clump giants with a small admixture of branch giants from the Gaia DR2 catalogue in a spatial cylinder with a rad…

2019 Astronomy Letters
Gaia 6
Poisson vs. Gaussian statistics for sparse X-ray data: Application to the soft X-ray spectrometer
DOI: 10.1093/pasj/psz053 Bibcode: 2019PASJ...71...75Y

Eckart, Megan E.; Kelley, Richard L.; Kilbourne, Caroline A. +8 more

Reliable results when fitting X-ray data require proper consideration of the statistics involved. We probe the impact of Gaussian versus Poisson statistics at low count levels using both the standard χ2 method and maximum likelihood based on Poisson (C) statistics. The difference is studied and quantified through simulated spectra with …

2019 Publications of the Astronomical Society of Japan
Hitomi 6
Radio observations of evaporating objects in the Cygnus OB2 region
DOI: 10.1051/0004-6361/201935179 Bibcode: 2019A&A...627A..58I

del Palacio, S.; Fernández-López, M.; Ishwara-Chandra, C. H. +2 more

We present observations of the Cygnus OB2 region obtained with the Giant Metrewave Radio Telescope (GMRT) at frequencies of 325 and 610 MHz. In this contribution we focus on the study of proplyd-like objects (also known as free-floating evaporating gas globules or frEGGs) that typically show an extended cometary morphology. We identify eight objec…

2019 Astronomy and Astrophysics
Gaia Herschel 6
Strongly magnetic Ap stars in the Gaia DR2 Hertzsprung-Russell diagram . I. Selecting the most reliable astrometric and photometric data
DOI: 10.1051/0004-6361/201935752 Bibcode: 2019A&A...628A..81S

Hubrig, S.; Chojnowski, S. Drew; Scholz, R. -D.

Context. Knowing the distribution of strongly magnetic Ap stars in the Hertzsprung-Russell diagram (HRD) allows us to study the evolution of their magnetic fields across the main sequence (MS). With a newly extended Ap star sample from APOGEE and available Gaia DR2 data, we can now critically review the results of previous studies based on HIPPARC…

2019 Astronomy and Astrophysics
Gaia Hipparcos 6