Search Publications

A Long-duration Luminous Type IIn Supernova KISS15s: Strong Recombination Lines from the Inhomogeneous Ejecta-CSM Interaction Region and Hot Dust Emission from Newly Formed Dust
DOI: 10.3847/1538-4357/aaff6b Bibcode: 2019ApJ...872..135K

Tominaga, Nozomu; Yoachim, Peter; Ivezić, Željko +7 more

We report the discovery of an SN 1988Z-like type IIn supernova KISS15s found in a low-mass star-forming galaxy at redshift z = 0.038 during the course of the Kiso Supernova Survey (KISS). KISS15s shows long-duration optical continuum and emission line light curves, indicating that KISS15s is powered by a continuous interaction between the expandin…

2019 The Astrophysical Journal
Gaia 19
J-PLUS: A wide-field multi-band study of the M 15 globular cluster. Evidence of multiple stellar populations in the RGB
DOI: 10.1051/0004-6361/201732441 Bibcode: 2019A&A...622A.179B

Cortesi, Arianna; Chies-Santos, Ana L.; Mendes de Oliveira, Claudia +21 more

Context. As a consequence of internal and external dynamical processes, Galactic globular clusters (GCs) have properties that vary radially. Wide-field observations covering the entire projected area of GCs out to their tidal radii (rtidal) can therefore give crucial information on these important relics of the Milky Way formation era. …

2019 Astronomy and Astrophysics
eHST 19
Electron Density Profiles in the Upper Ionosphere of Mars From 11 Years of MARSIS Data: Variability Due to Seasons, Solar Cycle, and Crustal Magnetic Fields
DOI: 10.1029/2018JA026327 Bibcode: 2019JGRA..124.3057D

Gurnett, D. A.; Morgan, D. D.; Halekas, J. +3 more

The Mars Advanced Radar for Subsurface and Ionosphere Sounding on board the Mars Express spacecraft measures the frequency of local plasma oscillations, which can be used to determine electron densities local to the spacecraft. This paper provides an overview of electron densities in the upper Martian ionosphere, obtained by investigating over 400…

2019 Journal of Geophysical Research (Space Physics)
MEx 19
Exploring the innermost dust formation region of the oxygen-rich AGB star IK Tauri with VLT/SPHERE-ZIMPOL and VLTI/AMBER
DOI: 10.1051/0004-6361/201834999 Bibcode: 2019A&A...628A.132A

Ohnaka, K.; Adam, C.

Context. Low- and intermediate-mass stars on the asymptotic giant branch (AGB) are known to be prevalent dust providers to galaxies, replenishing the surrounding medium with molecules and dust grains. However, the mechanisms responsible for the formation and acceleration of dust in the cool extended atmospheres of AGB stars are still open to debat…

2019 Astronomy and Astrophysics
Gaia ISO 19
Modeled Subglacial Water Flow Routing Supports Localized Intrusive Heating as a Possible Cause of Basal Melting of Mars' South Polar Ice Cap
DOI: 10.1029/2019JE006061 Bibcode: 2019JGRE..124.2101A

Butcher, F. E. G.; Balme, M. R.; Conway, S. J. +1 more

The discovery of an 20-km-wide area of bright subsurface radar reflections, interpreted as liquid water, beneath the Martian south polar layered deposits (SPLD) in data from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument, and the discovery of two geologically recent potential eskers (landforms produced by subgla…

2019 Journal of Geophysical Research (Planets)
MEx 19
The Filamentary Radio Lobes of the Seyfert-Starburst Composite Galaxy NGC 3079
DOI: 10.3847/1538-4357/ab371a Bibcode: 2019ApJ...883..189S

O'Dea, C. P.; Baum, S. A.; Kharb, P. +2 more

We present results from multifrequency polarization-sensitive Very Large Array observations of the Seyfert-starburst composite galaxy NGC 3079. Our sensitive radio observations reveal a plethora of radio “filaments” comprising the radio lobes in this galaxy. We analyze the origin of these radio filaments in the context of existing Chandra X-ray an…

2019 The Astrophysical Journal
eHST 19
Detection and Doppler monitoring of K2-285 (EPIC 246471491), a system of four transiting planets smaller than Neptune
DOI: 10.1051/0004-6361/201834001 Bibcode: 2019A&A...623A..41P

Kuzuhara, M.; Alonso, R.; Deeg, H. +43 more

Context. The Kepler extended mission, also known as K2, has provided the community with a wealth of planetary candidates that orbit stars typically much brighter than the targets of the original mission. These planet candidates are suitable for further spectroscopic follow-up and precise mass determinations, leading ultimately to the construction …

2019 Astronomy and Astrophysics
Gaia 19
Magnetic Field Strengths and Variations in Grain Alignment in the Local Bubble Wall
DOI: 10.3847/1538-4357/ab063c Bibcode: 2019ApJ...873...87M

Andersson, B. -G.; Medan, Ilija

Optical and infrared continuum polarization from the interstellar medium is known to generally be due to irregular dust grains aligned with the magnetic field. This provides an important tool to probe the geometry and strength of those fields, particularly if the variations in the grain alignment efficiencies can be understood. Here, we examine po…

2019 The Astrophysical Journal
Gaia 19
New online database of symbiotic variables: Symbiotics in X‑rays
DOI: 10.1002/asna.201913662 Bibcode: 2019AN....340..598M

Merc, J.; Gális, R.; Wolf, M.

Symbiotic variable stars belong to an interesting class of interacting binary systems. Since the beginning of this century, the systematic search for these objects has begun, and such surveys have led to discoveries of many new objects and dozens of candidates in the Milky Way and the Local Group. As the latest catalogue of symbiotic binaries is a…

2019 Astronomische Nachrichten
Gaia 19
Identifying transient and variable sources in radio images
DOI: 10.1016/j.ascom.2019.03.003 Bibcode: 2019A&C....27..111R

Eislöffel, J.; Wijers, R. A. M. J.; Fender, R. +16 more

With the arrival of a number of wide-field snapshot image-plane radio transient surveys, there will be a huge influx of images in the coming years making it impossible to manually analyse the datasets. Automated pipelines to process the information stored in the images are being developed, such as the LOFAR Transients Pipeline, outputting light cu…

2019 Astronomy and Computing
XMM-Newton 19