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Spatial Distribution of O VI Covering Fractions in the Simulated Circumgalactic Medium
DOI: 10.3847/1538-4357/abd033 Bibcode: 2021ApJ...907....8M

Charlton, Jane C.; Kacprzak, Glenn G.; Churchill, Christopher W. +6 more

We use adaptive mesh refinement cosmological simulations to study the spatial distribution and covering fraction of ${\rm{O}}\,{\rm\small{VI}}$ absorption in the circumgalactic medium (CGM) as a function of projected virial radius and azimuthal angle. We compare these simulations to an observed sample of 53 galaxies from the Multiphase Galaxy Halo…

2021 The Astrophysical Journal
eHST 4
The nature of bright C-complex asteroids
DOI: 10.1093/pasj/psaa118 Bibcode: 2021PASJ...73..240H

Hasegawa, Sunao; Usui, Fumihiko; Kuroda, Daisuke +1 more

Most C-complex asteroids have albedo values less than 0.1, but there are some high-albedo (bright) C-complex asteroids with albedo values exceeding 0.1. To reveal the nature and origin of bright C-complex asteroids, we conducted spectroscopic observations of the asteroids at visible and near-infrared wavelengths. As a result, the bright B-, C-, an…

2021 Publications of the Astronomical Society of Japan
AKARI 4
The Statistical Morphology of Saturn's Equatorial Energetic Neutral Atom Emission
DOI: 10.1029/2020GL091595 Bibcode: 2021GeoRL..4891595K

Mitchell, D. G.; Paranicas, C.; Badman, S. V. +6 more

Saturn's magnetosphere is an efficient emitter of energetic neutral atoms (ENAs), created through charge exchange of energetic ions with the extended neutral cloud originating from the icy moon Enceladus. We present an analysis using the complete image set captured by Cassini's Ion Neutral Camera to characterize Saturn's average ENA morphology. Co…

2021 Geophysical Research Letters
Cassini 4
The ROSAT Raster survey in the north ecliptic pole field. X-ray catalogue and optical identifications
DOI: 10.1051/0004-6361/202039476 Bibcode: 2021A&A...645A..95H

Moneti, A.; Hasinger, G.; Capak, P. +4 more

The north ecliptic pole (NEP) is an important region for extragalactic surveys. Deep and wide contiguous surveys are being performed by several space observatories, most currently with the eROSITA telescope. Several more are planned for the near future. We analyse all the ROSAT pointed and survey observations in a region of 40 deg2 arou…

2021 Astronomy and Astrophysics
Gaia XMM-Newton 4
A CO-to-H2 Ratio of ≈10-5 toward the Herbig Ae Star HK Ori
DOI: 10.3847/1538-3881/abea21 Bibcode: 2021AJ....161..217C

France, Kevin; Johns-Krull, Christopher M.; Cauley, P. Wilson +1 more

Measurements of gas mass in protoplanetary gas disks form the basis for estimating the conditions of planet formation. Among the most important constraints derived from disk diagnostics are the abundances of gas-phase species critical for understanding disk chemistry. Toward this end, we present direct line-of-sight measurements of H2 a…

2021 The Astronomical Journal
eHST 4
The first light curve solutions and period study of two contact binary systems: V1370 Tau and QQ Boo
DOI: 10.1016/j.newast.2020.101499 Bibcode: 2021NewA...8401499R

Davoudi, Fatemeh; Poro, Atila; Rahimi, Jabar +7 more

The first light curve solutions of the binary systems V1370 Tau and QQ Boo are presented. The periodic changes are calculated, and a new ephemeris presented for each of these two binary systems. O-C analysis is performed using the MCMC method in OCFit code. The changing rate of period was measured as dP/dt= 0.2423 days/year for V1370 Tau and dP/dt…

2021 New Astronomy
Gaia 4
Extremely Low Molecular Gas Content in the Vicinity of a Red Nugget Galaxy at z = 1.91
DOI: 10.3847/1538-4357/abd800 Bibcode: 2021ApJ...908..163M

Stiavelli, M.; Lucas, R. A.; D'Amato, Q. +3 more

We present Atacama Large Millimeter/submillimeter Array Band 5 observations of a galaxy at z = 1.91, GDS24569, in search of molecular gas in its vicinity via the [C I] 3P1-3P0 line. GDS24569 is a massive ( $\mathrm{log}{M}_{* }/{M}_{\odot }=11$ ), passively evolving galaxy, characterized by compact morph…

2021 The Astrophysical Journal
Herschel eHST 4
Study of UV-bright stellar populations in the globular cluster NGC 1261 using Astrosat
DOI: 10.1093/mnras/staa3758 Bibcode: 2021MNRAS.501.2140R

Rao, N. Kameswara; Sahu, Snehalata; Subramaniam, Annapurni +2 more

We present UV photometry of the globular cluster NGC 1261 using images acquired with the Ultraviolet Imaging Telescope (UVIT) on board Astrosat. We performed point-spread function (PSF) photometry on four near-UV (NUV) and two far-UV (FUV) images and constructed UV colour-magnitude diagrams (CMDs), in combination with the Hubble Space Telescope (H…

2021 Monthly Notices of the Royal Astronomical Society
Gaia eHST 4
Was Gale Crater (Mars) Connected to a Regionally Extensive Groundwater System?
DOI: 10.1029/2020GL092107 Bibcode: 2021GeoRL..4892107R

Horvath, D. G.; Roseborough, V.; Palucis, M. C.

Gale crater, home of the Curiosity rover, contains some of the best geomorphic and sedimentologic evidence on Mars for large lakes during the Hesperian and Amazonian. Orbital data and rover observations of delta deposits and terminations of gully networks suggest several phases of stable lake levels. However, the regional extent, water source (gro…

2021 Geophysical Research Letters
MEx 4
Arm Tangents and the Spiral Structure of the Milky Way—The Age Gradient
DOI: 10.4236/ijaa.2021.114022 Bibcode: 2021IJAA...11..445V

Vallée, Jacques P.

From the Sun, a look at the edge of each spiral arm in our Milky Way (seen tangentially, along the line of sight) can yield numerous insights. Using different arm tracers (dust, masers, synchrotron emission, CO gas, open star clusters), we observe here for the first time an age gradient (about 12 +/-2 Myrs/kpc), much as predicted by the density wa…

2021 International Journal of Astronomy and Astrophysics
Gaia 4