Search Publications

Absolute Properties of the Oscillating Eclipsing Algol X Trianguli
DOI: 10.3847/1538-3881/acbe9d Bibcode: 2023AJ....165..159L

Kim, Dong-Jin; Wolf, Marek; Hong, Kyeongsoo +2 more

We report results from the TESS photometric data and new high-resolution spectra of the Algol system X Tri showing short-period pulsations. From the echelle spectra, the radial velocities of the eclipsing pair were measured, and the rotational rate and effective temperature of the primary star were obtained to be v 1sini = 84 ± 6 km s

2023 The Astronomical Journal
Gaia 4
HOPS 361-C's Jet Decelerating and Precessing through NGC 2071 IR
DOI: 10.3847/1538-4357/acc401 Bibcode: 2023ApJ...948...39R

Quillen, Alice C.; Rubinstein, Adam E.; Federman, Samuel +5 more

We present a two-epoch Hubble Space Telescope study of NGC 2071 IR highlighting HOPS 361-C, a protostar producing an arced 0.2 parsec-scale jet. The proper motions for the brightest knots decrease from 350 to 100 km s-1 with increasing distance from the source. The [Fe II] and Paβ emission line intensity ratio gives a velocity jump thro…

2023 The Astrophysical Journal
eHST 4
Properties and asteroseismological analysis of a new ZZ ceti discovered by TMTS
DOI: 10.1093/mnras/stad1545 Bibcode: 2023MNRAS.523.1591G

Shi, Jianrong; Filippenko, Alexei V.; Esamdin, Ali +24 more

Tsinghua University-Ma Huateng Telescope for Survey (TMTS) aims to discover rapidly evolving transients by monitoring the northern sky. The TMTS catalogue is cross-matched with the white dwarf (WD) catalogue of Gaia EDR3, and light curves of more than a thousand WD candidates are obtained so far. Among them, the WD TMTS J23450729+5813146 is one in…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 4
Structure and Kinematics of Sh2-138-A Distant Hub-filament System in the Outer Galactic Plane
DOI: 10.3847/1538-4357/acb8bc Bibcode: 2023ApJ...944..228M

Baug, Tapas; Dewangan, Lokesh K.; Mallick, Kshitiz K. +2 more

We present a molecular line study of the Sh2-138 (IRAS 22308+5812) hub-filament system with the aim of investigating its structure and kinematics. Archival CO molecular line data from the Canadian Galactic Plane Survey (CO(J = 1-0)) for the wider region (~50' × 50') and the James Clerk Maxwell Telescope (CO(3-2), 13CO(3-2), and C18…

2023 The Astrophysical Journal
Herschel 4
The origin of ultramassive white dwarfs: hints from Gaia EDR3
DOI: 10.1093/mnras/stad068 Bibcode: 2023MNRAS.520..364F

Caiazzo, Ilaria; Heyl, Jeremy; Fleury, Leesa

Gaia Data Release 2 revealed a population of ultramassive white dwarfs on the Q branch that are moving anomalously fast for a local disc population with their young photometric ages. As the velocity dispersion of stars in the local disc increases with age, a proposed explanation of these white dwarfs is that they experience a cooling delay that ca…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 4
Spectral analysis of the Galactic supernova remnant Kesteven 69 with Suzaku
DOI: 10.1093/pasj/psad068 Bibcode: 2023PASJ...75.1273Y

Yamauchi, Shigeo; Pannuti, Thomas G.

The results of a Suzaku observation of the supernova remnant (SNR) Kesteven 69 = G21.8-0.6 are presented. To estimate the sky background precisely, we conducted a simultaneous fit of the source region spectrum with the background region spectrum and found that the SNR spectrum is well represented by a two-component ionizing plasma model composed o…

2023 Publications of the Astronomical Society of Japan
Suzaku 4
Coordinated X-ray and UV absorption within the accretion disk wind of the active galactic nucleus PG 1126-041
DOI: 10.1051/0004-6361/202244270 Bibcode: 2023A&A...679A..73G

Cappi, M.; Ponti, G.; Vignali, C. +14 more

Context. Accretion disk winds launched close to supermassive black holes (SMBHs) are a viable mechanism providing feedback between the SMBH and the host galaxy.
Aims: We aim to characterize the X-ray properties of the inner accretion disk wind of the nearby active galactic nucleus PG 1126-041 and to study its connection with the UV-absorbing …

2023 Astronomy and Astrophysics
XMM-Newton eHST 4
Quantifying Morphological Changes and Sediment Transport Pathways on Comet 67P/Churyumov-Gerasimenko
DOI: 10.1029/2022JE007723 Bibcode: 2023JGRE..12807723B

Vincent, J. -B.; Hayes, A. G.; Birch, S. P. D. +3 more

Comets are active geological worlds with primitive surfaces that have been shaped to varying degrees by sublimation-driven sediment transport and mass wasting processes. Rosetta's rendezvous with comet 67P/Churyumov-Gerasimenko (67P) in 2014 provided data with the necessary spatial and temporal resolutions to observe many evolutionary processes on…

2023 Journal of Geophysical Research (Planets)
Rosetta 4
Resolved low-J12CO excitation at 190 parsec resolution across NGC 2903 and NGC 3627
DOI: 10.1093/mnras/stad3091 Bibcode: 2023MNRAS.526.6347D

Chevance, M.; Dale, D. A.; Schinnerer, E. +14 more

The low-J rotational transitions of 12CO are commonly used to trace the distribution of molecular gas in galaxies. Their ratios are sensitive to excitation and physical conditions in the molecular gas. Spatially resolved studies of CO ratios are still sparse and affected by flux calibration uncertainties, especially since most do not ha…

2023 Monthly Notices of the Royal Astronomical Society
eHST JWST 4
The SOIR/Venus Express species concentration and temperature database: CO2, CO, H2O, HDO, H35Cl, H37Cl, HF individual and mean profiles
DOI: 10.1016/j.icarus.2023.115713 Bibcode: 2023Icar..40515713M

Vandaele, A. C.; Trompet, L.; Robert, S. +2 more

This work is an update of the SOIR mean and individual profiles of CO2, CO, H2O, HDO, H35Cl, H37Cl, HF, and the temperature measured at the Venus terminator during the Venus Express mission (2006-2014).

The previous versions of the database were published by Chamberlain et al. (2020); Mahieux et al.…

2023 Icarus
VenusExpress 4