Search Publications

SRG/eROSITA survey of Be stars
DOI: 10.1093/mnras/stad2399 Bibcode: 2023MNRAS.525.4186N

Nazé, Yaël; Robrade, Jan

Massive stars are known X-ray emitters and those belonging to the Be category are no exception. One type of X-ray emission even appears specific to that category, the γ Cas phenomenon. Its actual incidence has been particularly difficult to assess. Thanks to four semesters of sky survey data taken by the Spectrum-Roentgen-Gamma (SRG)/extended ROen…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 7
Grantecan spectroscopic observations and confirmations of planetary nebulae candidates in the Northern Galactic Plane
DOI: 10.1093/mnras/stac2896 Bibcode: 2023MNRAS.520..773R

Ritter, Andreas; Sabin, L.; Parker, Q. A. +3 more

We present Gran Telescopio Canarias (GTC) spectroscopic confirmations of 55 faint Planetary Nebulae (PNe) candidates discovered largely in the INT Photometric H α Survey (IPHAS) of the Northern Galactic Plane by our pro-am collaboration. We confirm 46 of them as 'True' (T), 4 as 'Likely' (L), and 5 as 'Possible' (P) PNe and including 5 new PNe cen…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 7
Reeling in the Whirlpool galaxy: Distance to M 51 clarified through Cepheids and the type IIP supernova 2005cs
DOI: 10.1051/0004-6361/202346971 Bibcode: 2023A&A...678A..44C

Leibundgut, B.; Anderson, R. I.; Blondin, S. +4 more

Context. The distance to the Whirlpool galaxy, M 51, is still debated, even though the galaxy has been studied in great detail. Current estimates range from 6.02 to 9.09 Mpc, and different methods yield discrepant results. No Cepheid distance has been published for M 51 to date.
Aims: We aim to estimate a more reliable distance to M 51 throug…

2023 Astronomy and Astrophysics
eHST 7
Surface chemical composition of single WNh stars
DOI: 10.1051/0004-6361/202347909 Bibcode: 2023A&A...680A..22M

Martins, Fabrice

Context. Wolf-Rayet (WR) stars of the WNh category contain a significant fraction of hydrogen at their surface. They can be hydrogen-burning, very massive stars or stars in a post-main sequence phase of evolution. Also, WNh stars are sometimes not included in population synthesis models.
Aims: We aim to better characterise the properties of s…

2023 Astronomy and Astrophysics
IUE 7
The Disturbed and Globular-cluster-rich Ultradiffuse Galaxy UGC 9050-Dw1
DOI: 10.3847/2041-8213/acf0c3 Bibcode: 2023ApJ...954L..39F

Sand, David J.; Jones, Michael G.; Fielder, Catherine E. +5 more

We investigate the ultradiffuse galaxy (UDG) UGC 9050-Dw1, which was selected because of its disturbed morphology as part of a larger sample of UDGs that display evidence for significant interactions. We use the Hubble Space Telescope's Advanced Camera for Surveys to identify globular clusters (GCs) associated with UGC 9050-Dw1, and the Jansky Ver…

2023 The Astrophysical Journal
eHST 7
On the Relation Between Jupiter's Aurora and the Dawnside Current Sheet
DOI: 10.1029/2023GL104123 Bibcode: 2023GeoRL..5004123X

Wei, Y.; Delamere, P. A.; Badman, S. V. +10 more

Jupiter's auroral emission is a spectacular phenomenon that provides insight into energy release processes related to the coupling of its magnetosphere and ionosphere. This energy release is influenced by solar wind conditions. Using joint observations from Juno and the Hubble Space Telescope (HST), we statistically investigate the relationship be…

2023 Geophysical Research Letters
eHST 7
Accurate mass-radius ratios for Hyades white dwarfs
DOI: 10.1093/mnras/stad1252 Bibcode: 2023MNRAS.522.3710P

Salaris, M.; Pasquini, L.; Pala, A. F. +4 more

We use the ESPRESSO spectrograph at the Very Large Telescope to measure velocity shifts and gravitational redshifts of eight bona fide Hyades white dwarfs, with an accuracy better than 1.5 per cent. By comparing the gravitational redshift measurements of the mass-to-radius ratio with the same ratios derived by fitting the Gaia photometry with theo…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 7
Catalog of the Galactic Population of X-Ray Pulsars in High-mass X-Ray Binary Systems
DOI: 10.3847/1538-4365/ace68f Bibcode: 2023ApJS..268...21K

Kim, Vitaliy; Izmailova, Ildana; Aimuratov, Yerlan

A catalog of the Galactic population of X-ray pulsars in high-mass X-ray binary (HMXB) systems is presented. It contains information about 82 confirmed sources: 18 persistent and 64 transient pulsars. Their basic parameters include spin period, spin evolution with global and local spin-up/spin-down and duration, orbital period, X-ray luminosity, m…

2023 The Astrophysical Journal Supplement Series
INTEGRAL 7
Relationships between energetic storm particle events and interplanetary shocks driven by full and partial halo coronal mass ejections
DOI: 10.1016/j.asr.2022.12.014 Bibcode: 2023AdSpR..71.2521A

Vainio, Rami; Valtonen, Eino; Al-Sawad, Amjad +1 more

We have analysed energetic storm particle (ESP) events in 116 interplanetary (IP) shocks driven by front-side full and partial halo coronal mass ejections (CMEs) with speeds > 400 km s-1during the years 1996-2015. We investigated the occurrence and relationships of ESP events with several parameters describing the IP shocks, and the …

2023 Advances in Space Research
SOHO 7
An emerging and enigmatic spectral class of isolated DAe white dwarfs
DOI: 10.1093/mnras/stad2171 Bibcode: 2023MNRAS.524.4996E

Hermes, J. J.; Munday, James; Gänsicke, Boris T. +9 more

Two recently discovered white dwarfs, WD J041246.84 + 754942.26 and WD J165335.21 - 100116.33, exhibit Hα and Hβ Balmer line emission similar to stars in the emerging DAHe class, yet intriguingly have not been found to have detectable magnetic fields. These white dwarfs are assigned the spectral type DAe. We present detailed follow-up of the two k…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 7