Search Publications

Heterogeneous evolution of the Galaxy and the origin of the short-lived nuclides in the early solar system
DOI: 10.1093/mnras/stz2720 Bibcode: 2019MNRAS.490.1620K

Kaur, Tejpreet; Sahijpal, Sandeep

We present Galactic chemical evolution (GCE) models of the short-lived radionuclides (SLRs), 26Al, 36Cl, 41Ca, 53Mn, and 60Fe, across the entire Milky Way galaxy. The objective is to understand the spatial and temporal distribution of the SLRs in the galaxy. The gamma-ray observations infer wi…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 7
Vertical and horizontal heterogeneity of atmospheric dust loading in northern Gale Crater, Mars
DOI: 10.1016/j.icarus.2019.03.041 Bibcode: 2019Icar..329..197M

Lemmon, Mark T.; Newman, Claire E.; Moore, Casey A. +3 more

This paper updates the record of atmospheric dust loading within northern Gale Crater, Mars, by providing line-of-sight extinction (LOS-Ext) measurements of the intervening dust between the rover and the crater rim. These measurements are derived from images taken with the Navigation Cameras (Navcam) onboard the Mars Science Laboratory (MSL) rover…

2019 Icarus
MEx 7
Characteristics of the Solar Coronal Line Profiles from Fabry-Perot Interferometric Observations
DOI: 10.1007/s11207-019-1409-7 Bibcode: 2019SoPh..294...26P

Chandrasekhar, T.; Raju, K. P.; Prabhakar, Maya

This article reports the analysis of a set of Fabry-Perot interferograms that were studied to probe the physical parameters of the inner solar corona. The observations were carried out in the coronal green line, Fe XIV 5302.86 Å, during the total solar eclipse of 21 June 2001 that occurred in Lusaka, Zambia. The study was performed in the radial r…

2019 Solar Physics
SOHO 7
The Enhancement of the Energetic Particle Intensities in ICMEs
DOI: 10.3847/1538-4357/ab4596 Bibcode: 2019ApJ...885...54X

Li, Gang; Wang, Yuming; Shen, Chenglong +5 more

The behavior of energetic particles in interplanetary coronal mass ejections (ICMEs) is of great interest. In general, due to the relatively closed magnetic structures of ICMEs, the energetic-particle intensities are usually depressed in them. However, previous studies have found some counterexamples. In this work, using protons with energies form…

2019 The Astrophysical Journal
SOHO 7
Analysis of a long-lived, two-cell lightning storm on Saturn
DOI: 10.1051/0004-6361/201833014 Bibcode: 2019A&A...621A.113F

Gurnett, D. A.; Kurth, W. S.; Delcroix, M. +4 more

Lightning storms in Saturn's atmosphere can last for a few days up to several months. In this paper we analyze a lightning storm that raged for seven and a half months at a planetocentric latitude of 35° south from the end of November 2007 until mid-July 2008. Thunderstorms observed by the Cassini spacecraft before this time were characterized by …

2019 Astronomy and Astrophysics
Cassini 7
Dwarf Spheroidal Galaxies in the M101 Group and Behind it
DOI: 10.1007/s10511-019-09582-7 Bibcode: 2019Ap.....62..293K

Karachentsev, I. D.; Makarova, L. N.

We use images from the Hubble Space Telescope to determine the distances to a dozen objects with low surface brightness recently observed around the bright nearby spiral M101. Only two dwarf galaxies, M101-DwA and M101-Dw9, turn out to be actual satellites of M101 at distances of about 7 Mpc. The other objects are probably members of a distant gro…

2019 Astrophysics
eHST 7
Principal component analysis of up-the-ramp sampled infrared array data
DOI: 10.1117/1.JATIS.5.2.028001 Bibcode: 2019JATIS...5b8001R

Rauscher, Bernard J.; Arendt, Richard G.; Fixsen, Dale J. +3 more

We describe the results of principal component analysis (PCA) of up-the-ramp sampled infrared (IR) array data from the Hubble Space Telescope wide field camera 3 (WFC3 IR), James Webb Space Telescope NIRSpec, and prototype Wide Field Infrared Survey Telescope's wide field instrument detectors. These systems use, respectively, Teledyne H1R, H2RG, a…

2019 Journal of Astronomical Telescopes, Instruments, and Systems
eHST 7
Search for multiwavelength emission from the binary millisecond pulsar PSR J1836-2354A in the globular cluster M22
DOI: 10.1093/mnras/stz1100 Bibcode: 2019MNRAS.486.3992A

de Martino, D.; Di Salvo, T.; Iaria, R. +5 more

We present a multiband search for X-ray, optical, and γ-ray emission of the radio binary millisecond pulsar J1836-2354A, hosted in the globular cluster M22. X-ray emission is significantly detected in two Chandra observations, performed in 2005 and 2014, at a luminosity of ∼2-3 × 1030 erg s-1, in the 0.5-8 keV energy range. T…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 7
Monitoring of the D doublet of neutral sodium during transits of two `evaporating' planets
DOI: 10.1093/mnras/stz693 Bibcode: 2019MNRAS.485.3876G

Hirano, T.; Ansdell, M.; Gaidos, E.

Spectroscopic transit detection of constituents in winds from `evaporating' planets on close-in transiting orbits could provide desperately needed information on the composition, formation, and orbital evolution of such objects. We obtained high-resolution optical spectra of the host stars during a single transit of Kepler-1520b and two transits o…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 7
Understanding the Plasma and Magnetic Field Evolution of a Filament Using Observations and Nonlinear Force-free Field Modeling
DOI: 10.3847/1538-4357/ab54d2 Bibcode: 2019ApJ...887..240Y

Savcheva, Antonia; van Driel-Gesztelyi, Lidia; Green, Lucie M. +4 more

We present observations and magnetic field models of an intermediate filament present on the Sun in 2012 August, associated with a polarity inversion line that extends from AR 11541 in the east into the quiet Sun at its western end. A combination of Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly, SDO/Helioseismic and Magnetic Imager…

2019 The Astrophysical Journal
SOHO 7