Search Publications

A Global and Seasonal Perspective of Martian Water Vapor From ExoMars/NOMAD
DOI: 10.1029/2021JE006878 Bibcode: 2021JGRE..12606878C

Aoki, S.; Vandaele, A. C.; Daerden, F. +18 more

Slightly less than a Martian Year of nominal science (March 2018-January 2020) with the ExoMars Trace Gas Orbiter has furthered the ongoing investigation of dayside water vapor column abundance. These dayside observations span latitudes between 75°S and 75°N, and all longitudes, which can provide global snapshots of the total water column abundanc…

2021 Journal of Geophysical Research (Planets)
ExoMars-16 14
An approximate analytic solution to the coupled problems of coronal heating and solar-wind acceleration
DOI: 10.1017/S0022377821000052 Bibcode: 2021JPlPh..87c9004C

Chandran, Benjamin D. G.

Between the base of the solar corona at $r=r_\textrm {b}$ and the Alfvén critical point at $r=r_\textrm {A}$, where $r$ is heliocentric distance, the solar-wind density decreases by a factor $ \mathop > \limits_∼ 10^5$, but the plasma temperature varies by a factor of only a few. In this paper, I show that such quasi-isothermal evolution out to…

2021 Journal of Plasma Physics
Ulysses 14
Optical spectroscopy of Galactic field classical Be stars
DOI: 10.1093/mnras/staa3469 Bibcode: 2021MNRAS.500.3926B

Mathew, Blesson; Paul, K. T.; Subramaniam, Annapurni +3 more

In this study, we analyse the emission lines of different species present in 118 Galactic field classical Be stars in the wavelength range of 3800-9000 Å. We re-estimated the extinction parameter (AV) for our sample stars using the newly available data from Gaia DR2 and suggest that it is important to consider AV while measur…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 14
A Broadband X-Ray View of the Precessing Accretion Disk and Pre-eclipse Dip in the Pulsar Her X-1 with NuSTAR and XMM-Newton
DOI: 10.3847/1538-4357/abe122 Bibcode: 2021ApJ...909..186B

Pottschmidt, Katja; Staubert, Rüdiger; Wilms, Jörn +5 more

We present a broadband X-ray timing study of the variations in pulse behavior with the superorbital cycle in the low-mass X-ray binary Her X-1. This source shows a 35 day superorbital modulation in X-ray flux that is likely caused by occultation by a warped, precessing accretion disk. Our data set consists of four joint XMM-Newton and NuSTAR obser…

2021 The Astrophysical Journal
XMM-Newton 14
A global investigation of wrinkle ridge formation events; Implications towards the thermal evolution of Mars
DOI: 10.1016/j.icarus.2021.114625 Bibcode: 2021Icar..36914625R

Ruj, Trishit; Kawai, Kenji

Wrinkle ridges (WR) are well-established paleo-stress indicators providing information on the compressional history and thermal evolution of Mars. Therefore, constraining their timing of formation on a global scale could yield better insight into the tectonic history, evolution of the mantle, and the paleoclimate of the planet. Here, we have updat…

2021 Icarus
MEx 14
A principal component analysis of polycyclic aromatic hydrocarbon emission in NGC 2023
DOI: 10.1093/mnras/staa3175 Bibcode: 2021MNRAS.500..177S

Cami, Jan; Peeters, Els; Sidhu, Ameek +1 more

We use the measured fluxes of polycyclic aromatic hydrocarbon (PAH) emission features at 6.2, 7.7, 8.6, 11.0, and 11.2 µm in the reflection nebula NGC 2023 to carry out a principal component analysis (PCA) as a means to study previously reported variations in the PAH emission. We find that almost all of the variations (99 per cent) can be ex…

2021 Monthly Notices of the Royal Astronomical Society
Herschel 14
Infrared spectropolarimetric detection of intrinsic polarization from a core-collapse supernova
DOI: 10.1038/s41550-021-01320-4 Bibcode: 2021NatAs...5..544T

Tinyanont, Samaporn; Leonard, Douglas C.; De, Kishalay +8 more

Massive stars die an explosive death as a core-collapse supernova (CCSN). The exact physical processes that cause the collapsing star to rebound into an explosion are not well understood1-3, and the key to resolving this issue may lie in the measurement of the shape of CCSNe ejecta. Spectropolarimetry is the only way to perform this mea…

2021 Nature Astronomy
eHST 14
KCWI Observations of the Extended Nebulae in Mrk 273
DOI: 10.3847/1538-4357/abf4da Bibcode: 2021ApJ...914...17L

Leung, Gene C. K.; Coil, Alison L.; Perrotta, Serena +1 more

Ultraluminous infrared galaxies (ULIRGs) represent a critical stage in the merger-driven evolution of galaxies when active galactic nucleus (AGN) activity is common and AGN feedback is expected. We present high-sensitivity and large field-of-view integral field spectroscopy of the ULIRG Mrk 273 using new data from the Keck Cosmic Web Imager (KWCI)…

2021 The Astrophysical Journal
eHST 14
Three faint-source microlensing planets detected via the resonant-caustic channel
DOI: 10.1051/0004-6361/202141517 Bibcode: 2021A&A...655A..21H

Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk +32 more


Aims: We conducted a project of reinvestigating the 2017-2019 microlensing data collected by high-cadence surveys with the aim of finding planets that were missed due to the deviations of planetary signals from the typical form of short-term anomalies.
Methods: The project led us to find three planets, KMT-2017-BLG-2509Lb, OGLE-2017-BLG-…

2021 Astronomy and Astrophysics
eHST 14
HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure
DOI: 10.3847/1538-4357/ac0cf2 Bibcode: 2021ApJ...918...39L

Kwon, Woojin; Fissel, Laura M.; Li, Di +14 more

We present a study of the relative orientation between the magnetic field and elongated cloud structures for the ρ Oph A and ρ Oph E regions in L1688 in the Ophiuchus molecular cloud. Combining inferred magnetic field orientation from HAWC+ 154 µm observations of polarized thermal emission with column density maps created using Herschel subm…

2021 The Astrophysical Journal
Herschel 14