Search Publications

Monitoring observations of SMC X-1's excursions (MOOSE)-I. Programme description and initial high state spectral results
DOI: 10.1093/mnras/stac1674 Bibcode: 2022MNRAS.514.5457D

Clarkson, William I.; Dage, Kristen C.; Bahramian, Arash +8 more

SMC X-1 has exhibited three superorbital period excursions since the onset of X-ray monitoring beginning with the Rossi X-ray Timing Explorer's launch in 1995. TheNeutron star Interior Composition Explorer has recently probed a fourth observed excursion beginning in 2021 with our programme monitoring observations of SMC X-1's excursions (MOOSE). T…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
A Highway for Atmospheric Ion Escape from Earth during the Impact of an Interplanetary Coronal Mass Ejection
DOI: 10.3847/1538-4357/ac8a93 Bibcode: 2022ApJ...937....4Z

Zong, Qiugang; Xie, Lun; Zhang, Hui +9 more

A single satellite hardly measures the overall ion escape rate from a planet. Therefore, the question concerning the long-term atmospheric evolution of whether a planetary magnetic field protects its atmosphere or aggravates atmospheric loss remains unresolved. Here, combined data from multiple platforms including Cluster, DMSP, IMAGE, and Polar s…

2022 The Astrophysical Journal
Cluster 4
A detailed star formation history for the extremely diffuse Andromeda XIX dwarf galaxy
DOI: 10.1093/mnras/stac2794 Bibcode: 2022MNRAS.517.4382C

Williams, Benjamin F.; Gilbert, Karoline M.; Dolphin, Andrew +3 more

We present deep imaging of the ultradiffuse Andromeda XIX dwarf galaxy from the Advance Camera for Surveys on the Hubble Space Telescope which resolves its stellar populations to below the oldest main-sequence turn-off. We derive a full star formation history for the galaxy using MATCH, and find no evidence of star formation in the past 8 Gyr. We …

2022 Monthly Notices of the Royal Astronomical Society
eHST 4
COol Companions ON Ultrawide orbiTS (COCONUTS). III. A Very Red L6 Benchmark Brown Dwarf around a Young M5 Dwarf
DOI: 10.3847/1538-4357/ac7ce9 Bibcode: 2022ApJ...935...15Z

Magnier, Eugene A.; Shappee, Benjamin J.; Morley, Caroline V. +5 more

We present the third discovery from the COol Companions ON Ultrawide orbiTS (COCONUTS) program, the COCONUTS-3 system, composed of the young M5 primary star UCAC4 374-046899 and the very red L6 dwarf WISEA J081322.19-152203.2. These two objects have a projected separation of $61^{\prime\prime} $ (1891 au) and are physically associated given their …

2022 The Astrophysical Journal
Gaia 4
Impact ionization dust detection with compact, hollow and fluffy dust analogs
DOI: 10.1016/j.pss.2022.105536 Bibcode: 2022P&SS..22005536H

Srama, R.; Pommerol, A.; Hornung, K. +14 more

Impact ionization of high-velocity cosmic dust particles has been used as a basic principle for dust detectors in space for many decades. It has provided optimum means to gain insight into the dust environment in the solar system. The Ulysses Dust Detector System provided for the first time impact ionization-based detection of interstellar dust (I…

2022 Planetary and Space Science
Ulysses 4
XMM-Newton discovery of very high obscuration in the candidate supergiant fast X-ray transient AX J1714.1-3912
DOI: 10.1093/mnras/stac691 Bibcode: 2022MNRAS.512.2929S

Sidoli, L.; Esposito, P.; Polletta, M. +2 more

We have analysed an archival XMM-Newton EPIC observation that serendipitously covered the sky position of a variable X-ray source AX J1714.1-3912, previously suggested to be a supergiant fast X-ray transient (SFXT). During the XMM-Newton observation the source is variable on a time-scale of hundred seconds and shows two luminosity states, with a f…

2022 Monthly Notices of the Royal Astronomical Society
Gaia INTEGRAL XMM-Newton 4
Timing and spectral studies of the X-ray pulsar 2S 1417–624 during the outburst in 2021
DOI: 10.1007/s10509-022-04150-6 Bibcode: 2022Ap&SS.367..112M

Mandal, Manoj; Pal, Sabyasachi

We study the timing and spectral properties of the X-ray pulsar 2S 1417–624 during the recent outburst in January 2021 based on the Neutron Star Interior Composition Explorer (NICER) observation. We also used some early data from the 2018 outburst to compare different temporal and spectral properties. The evolution of the spin period and pulsed fl…

2022 Astrophysics and Space Science
Gaia 4
The Star Formation-Gas Density Relation in Four Galactic GMCs: Effects of Stellar Feedback
DOI: 10.3847/1538-4357/ac9054 Bibcode: 2022ApJ...938..145B

Bieging, John H.; Kong, Shuo

We present maps of four Galactic giant molecular clouds (GMCs) in the J = 2-1 emission of both CO and 13CO. We use an LTE analysis to derive maps of the CO excitation temperature and column density and the distribution of total molecular gas column density, Σgas. The depletion of CO by freeze-out onto cold dust grains is acco…

2022 The Astrophysical Journal
Gaia 4
A probabilistic method for detecting solar-like oscillations using meaningful prior information. Application to TESS 2-minute photometry
DOI: 10.1051/0004-6361/202243064 Bibcode: 2022A&A...663A..51N

Chaplin, W. J.; Davies, G. R.; Nielsen, M. B. +2 more

Context. Current and future space-based observatories such as the Transiting Exoplanet Survey Satellite (TESS) and PLATO are set to provide an enormous amount of new data on oscillating stars, and in particular stars that oscillate similar to the Sun. Solar-like oscillators constitute the majority of known oscillating stars and so automated analys…

2022 Astronomy and Astrophysics
Gaia 4
Constraining Global Solar Models through Helioseismic Analysis
DOI: 10.3847/1538-4357/ac7a44 Bibcode: 2022ApJ...934..161S

Kosovichev, Alexander G.; Stejko, Andrey M.; Guerrero, Gustavo +4 more

Global hydrodynamic simulations of internal solar dynamics have focused on replicating the conditions for solar-like (equator rotating faster than the poles) differential rotation and meridional circulation using the results of helioseismic inversions as a constraint. Inferences of meridional circulation, however, have provided controversial resul…

2022 The Astrophysical Journal
SOHO 4