Search Publications

Further Studies of the Association of Planetary Nebula BMP J16135406 with Galactic Open Cluster NGC 6067
DOI: 10.3390/galaxies10020044 Bibcode: 2022Galax..10...44F

Parker, Quentin A.; Sabin, Laurence; Zijlstra, Albert A. +3 more

Planetary Nebulae (PNe) that are physical members of Galactic open clusters are powerful probes that allow precise determination of their distance and crucially their initial mass on the main sequence. Here, we revisit the physical association of the PN BMP J1613–5406 with the open cluster NGC 6067 and present our preliminary results based on our …

2022 Galaxies
Gaia 4
Mass assembly history of dark matter haloes in the light of H0 tension
DOI: 10.1093/mnras/stac129 Bibcode: 2022MNRAS.511.1601K

Kameli, Hamed; Baghram, Shant

The Hubble tension may introduce a new course of action to revise the standard Lambda cold dark matter (ΛCDM) model to unravel dark energy and dark matter physics. The Hubble parameter can be reconstructed by late-time observations of the background evolution model independently. We relate the reconstructed Hubble parameter to the structure format…

2022 Monthly Notices of the Royal Astronomical Society
eHST 4
Understanding the physical state of hot plasma formed through stellar wind collision in WR140 using high-resolution X-ray spectroscopy
DOI: 10.1093/mnras/stac1289 Bibcode: 2022MNRAS.513.6074M

Hamaguchi, Kenji; Miyamoto, Asca; Sugawara, Yasuharu +5 more

We analyse a series of XMM-Newton RGS data of the binary Wolf-Rayet star WR140 that encompasses one entire orbit. We find that the RGS detects X-rays from optically thin thermal plasma only during orbital phases when the companion O star is on the near side of the WR star. Although such X-rays are believed to be emitted from the shock cone formed …

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Local-time Dependence of Chemical Species in the Venusian Mesosphere
DOI: 10.3847/PSJ/ac3bd3 Bibcode: 2022PSJ.....3....3S

Shao, Wencheng D.; Zhang, Xi; Mendonça, João +1 more

Observed chemical species in the Venusian mesosphere show local-time variabilities. SO2 at the cloud top exhibits two local maxima over local time, H2O at the cloud top is uniformly distributed, and CO in the upper atmosphere shows a statistical difference between the two terminators. In this study, we investigated these loca…

2022 The Planetary Science Journal
VenusExpress 4
Substellar Hyades Candidates from the UKIRT Hemisphere Survey
DOI: 10.3847/1538-3881/ac5f50 Bibcode: 2022AJ....163..242S

Cushing, Michael C.; Schneider, Adam C.; Faherty, Jacqueline K. +14 more

We have used data from the UKIRT Hemisphere Survey to search for substellar members of the Hyades cluster. Our search recovered several known substellar Hyades members, and two known brown dwarfs that we suggest may be members based on a new kinematic analysis. We uncovered thirteen new substellar Hyades candidates, and obtained near-infrared foll…

2022 The Astronomical Journal
Gaia 4
Searching for giant planets in the outer Solar system with far-infrared all-sky surveys
DOI: 10.1093/mnras/stac2044 Bibcode: 2022MNRAS.515.4828S

Serjeant, Stephen; Sedgwick, Chris

We have explored a method for finding giant planets in the outer Solar system by detecting their thermal emission and proper motion between two far-infrared all-sky surveys separated by 23.4 yr, taken with the InfraRed Astronomical Satellite (IRAS) and the AKARI Space Telescope. An upper distance limit of about 8000 AU is given by both the sensiti…

2022 Monthly Notices of the Royal Astronomical Society
AKARI 4
Differential Proper Motion Spin of the Hipparcos and Gaia Celestial Reference Frames
DOI: 10.3847/1538-3881/ac88d1 Bibcode: 2022AJ....164..157M

Makarov, Valeri V.

The Hipparcos catalog provides the first epoch of the celestial reference frame (CRF) in the optical domain and serves as an indispensable tool to verify and improve the Gaia CRF for the brighter stars (V < 11 mag) and to identify the elusive astrometric binary stars with dim or invisible companions, including long-period exoplanets. The system…

2022 The Astronomical Journal
Gaia Hipparcos 4
SDSS-IV MaNGA: Identification and multiwavelength properties of Type-1 AGN in the DR15 sample
DOI: 10.1093/mnras/stac1505 Bibcode: 2022MNRAS.514.3626C

Negrete, C. A.; Hernández-Toledo, H. M.; Ibarra-Medel, H. +2 more

We present a method to identify type-1 active galactic nuclei (AGNs) in the central 3 arcsec integrated spectra of galaxies in the MaNGA DR15 sample. It is based on flux ratios estimates in spectral bands flanking the expected H α broad component H αBC. The high signal-to-noise ratio obtained (mean S/N = 84) permits the identification o…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Revising Properties of Planet-Host Binary Systems. II. Apparent Near-Earth-analog Planets in Binaries Are Often Sub-Neptunes
DOI: 10.3847/1538-3881/ac89ed Bibcode: 2022AJ....164..138S

Kraus, Adam L.; Sullivan, Kendall

Identifying rocky planets in or near the habitable zones of their stars (near-Earth analogs) is one of the key motivations of many past and present planet-search missions. The census of near-Earth analogs is important because it informs calculations of the occurrence rate of Earth-like planets, which in turn feed into calculations of the yield of …

2022 The Astronomical Journal
Gaia 4
The changing-look AGN NGC 1566 in quiescence with XMM-Newton: a nuclear starburst and an AGN competing in power?
DOI: 10.1093/mnras/stac1312 Bibcode: 2022MNRAS.514..403T

Santos-Lleó, M.; Ballo, L.; Jiménez Bailón, E. +8 more

Star formation accretion on to the super massive black holes (SMBHs) and feedback processes link the evolution of galaxies with their SMBHs. X-ray observations in the imaging and spectral regime have revealed to be an important tool to study the connection between nuclear activity and circumnuclear star formation in nearby active galactic nuclei (…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4