Search Publications

A Geoeffective CME Caused by the Eruption of a Quiescent Prominence on 29 September 2013
DOI: 10.1007/s11207-020-01619-x Bibcode: 2020SoPh..295...55G

Grechnev, V. V.; Kuzmenko, I. V.

The eruption of a large prominence that occurred away of active regions in the SOL2013-09-29 event produced a fast coronal mass ejection (CME) and a shock wave. The event caused considerable geospace disturbances, including a proton enhancement that have been addressed in previous studies. Continuing with the analysis of this event, we focus on th…

2020 Solar Physics
SOHO 7
A broadband X-ray view of the NLSy1 1E 0754.6+3928
DOI: 10.1051/0004-6361/201936701 Bibcode: 2020A&A...635A..18M

Bianchi, S.; Petrucci, P. -O.; Miniutti, G. +8 more

Context. The soft X-ray band of many active galactic nuclei (AGNs) is affected by obscuration due to partially ionised matter crossing our line of sight. In this context, two past XMM-Newton observations that were six months apart and a simultaneous NuSTAR-Swift exposure of the Narrow Line Seyfert 1 galaxy 1E 0754.6+3928, which was approximately e…

2020 Astronomy and Astrophysics
XMM-Newton 7
Determination of the Configurations of Boundaries in Space
DOI: 10.1029/2020JA028163 Bibcode: 2020JGRA..12528163S

Russell, C. T.; Dunlop, M.; Rong, Zhaojin +5 more

This research aims to determine the geometrical configurations of boundary surfaces in the space environment, based on multiple spacecraft measurements. To achieve this, the Normal Field Analysis (NFA) method is presented here. With multipoint observations, the three-dimensional gradient of the normal of boundary layers can be obtained, and the pr…

2020 Journal of Geophysical Research (Space Physics)
Cluster 7
Gaia DR2 data and the evolutionary status of eight high-velocity hot post-AGB candidates
DOI: 10.1093/pasj/psaa097 Bibcode: 2020PASJ...72...99P

Matsuno, Tadafumi; Aoki, Wako; Parthasarathy, Mudumba

From Gaia DR2 data of eight high-velocity hot post-AGB candidates, LS 3593, LSE 148, LS 5107, HD 172324, HD 214539, LS IV -12 111, LS III +52 24, and LS 3099, we found that six of them have accurate parallaxes which made it possible to derive their distances, absolute visual magnitudes (MV) and luminosity (log L/L). All the …

2020 Publications of the Astronomical Society of Japan
Gaia 7
Properties of F Stars with Stable Radial Velocity Timeseries: A Useful Metric for Selecting Low-jitter F Stars
DOI: 10.3847/1538-3881/ab775c Bibcode: 2020AJ....159..236L

Wright, Jason T.; Isaacson, Howard; Luhn, Jacob K.

In a companion paper, we have conducted an in-depth analysis of radial velocity jitter of over 600 stars, examining the astrophysical origins including stellar granulation, oscillation, and magnetic activity. In this paper, we highlight a subsample of those stars, specifically the main sequence and "retired" F stars -- which we refer to as "MSRF" …

2020 The Astronomical Journal
Gaia 7
A HaloSat Analysis of the Cygnus Superbubble
DOI: 10.3847/1538-4357/abc41b Bibcode: 2020ApJ...905...91B

Kaaret, Philip; Kuntz, K. D.; Bluem, Jesse +5 more

The Cygnus Superbubble (CSB) is a region of soft X-ray emission approximately 13 degrees wide in the direction of the local spiral arm. Such a large region might be the result of strong stellar winds and supernovae from nearby stellar nurseries, or it could be the result of a single event—a hypernova. HaloSat observed four nonoverlapping 10 degree…

2020 The Astrophysical Journal
Gaia 6
A Mystery in Chamaeleon: Serendipitous Discovery of a Galactic Symbiotic Nova
DOI: 10.3847/1538-3881/aba435 Bibcode: 2020AJ....160..125L

Ting, Yuan-Sen; Greene, Jenny E.; Pope, Benjamin J. S. +3 more

We present the serendipitous discovery of a low optical-luminosity nova occurring in a D-type symbiotic binary star system in the Milky Way. We lay out the extensive archival data alongside new follow-up observations related to the stellar object CN Cha in the constellation of Chamaeleon. The object had long period (250 days), high amplitude (3 ma…

2020 The Astronomical Journal
AKARI Gaia 6
Dust emission, extinction, and scattering in LDN 1642
DOI: 10.1051/0004-6361/202038611 Bibcode: 2020A&A...643A.132J

Ysard, Nathalie; Juvela, Mika; Neha, Sharma +3 more

Context. LDN 1642 is a rare example of a star-forming, high-latitude molecular cloud. The dust emission of LDN 1642 has already been studied extensively in the past, but its location also makes it a good target for studies of light scattering.
Aims: We wish to study the near-infrared (NIR) light scattering in LDN 1642, its correlation with th…

2020 Astronomy and Astrophysics
Gaia Herschel 6
On the Effects of UV Photons/X-Rays on the Chemistry of the Sgr B2 Cloud
DOI: 10.3847/1538-4357/ab8d34 Bibcode: 2020ApJ...895...57A

Martín-Pintado, J.; Requena-Torres, M. A.; Llerena, M. +7 more

The lines of HOC+, HCO, and CO+ are considered good tracers of photon-dominated regions (PDRs) and X-ray-dominated regions. We study these tracers toward regions of the Sgr B2 cloud selected to be affected by different heating mechanisms. We find the lowest values of the column density ratios of HCO+ versus HOC

2020 The Astrophysical Journal
XMM-Newton 6
A Galactic dust devil: far-infrared observations of the Tornado supernova remnant candidate
DOI: 10.1093/mnras/staa2925 Bibcode: 2020MNRAS.499.5665C

De Looze, I.; Rho, J.; Dunne, L. +10 more

We present complicated dust structures within multiple regions of the candidate supernova remnant (SNR) the 'Tornado' (G357.7-0.1) using observations with Spitzer and Herschel. We use point process mapping, PPMAP, to investigate the distribution of dust in the Tornado at a resolution of 8 arcsec, compared to the native telescope beams of 5-36 arcs…

2020 Monthly Notices of the Royal Astronomical Society
Herschel XMM-Newton 6