Search Publications

Probing the accretion geometry of the atoll source 4U 1702-429 in different spectral states with NICER, NuSTAR, and AstroSat
DOI: 10.1093/mnras/stae541 Bibcode: 2024MNRAS.529.4311B

Homan, Jeroen; Banerjee, Srimanta

We perform a comprehensive spectral study of a carefully selected sample (total exposure ~50.5 ks) of NICER observations of the atoll neutron star low-mass X-ray binary 4U 1702-429. Our sample encompasses nearly all classical spectral states found within the NICER data set. We require two thermal emission components, originating from the accretion…

2024 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 3
Surveys of clumps, cores, and condensations in Cygnus-X. Searching for circumstellar disks
DOI: 10.1051/0004-6361/202346763 Bibcode: 2024A&A...684A.141P

Qiu, Keping; Cao, Yue; Yang, Kai +2 more

Context. Theories and models have suggested that circumstellar disks could channel material to the central protostar, and resist star formation feedback. Our current knowledge of the picture and role of disks around massive protostars is unclear because the observational evidence of these circumstellar disks is limited.
Aims: To investigate w…

2024 Astronomy and Astrophysics
Herschel 3
Testing the asteroseismic estimates of stellar radii with surface brightness-colour relations and Gaia DR3 parallaxes: Red giants and red clump stars
DOI: 10.1051/0004-6361/202451473 Bibcode: 2024A&A...690A.327V

Valle, G.; Dell'Omodarme, M.; Prada Moroni, P. G. +1 more

Aims. We compared stellar radii derived from asteroseismic scaling relations with those estimated using two independent surface brightness-colour relations (SBCRs) combined with Gaia DR3 parallaxes. Methods. We cross-matched asteroseismic and astrometric data for over 6400 red giant branch (RGB) and red clump (RC) stars from the APO-K2 catalogue w…

2024 Astronomy and Astrophysics
Gaia 3
Double-lined Spectroscopic Binaries from the LAMOST Low-resolution Survey
DOI: 10.3847/1538-4365/ad856a Bibcode: 2024ApJS..275...40L

Ting, Yuan-Sen; Liu, Junhui; Zhang, Bo +1 more

We report on a data-driven spectral model that we have developed for the identification of double-lined spectroscopic binary stars (SB2s) in the Large Sky Area Multi-Object fiber Spectroscopic Telescope low-resolution survey (R ∼ 1800). Employing simultaneous fitting with both single-star and binary-star models, we detected over 4800 SB2 candidate…

2024 The Astrophysical Journal Supplement Series
Gaia 3
A survey for variable young stars with small telescopes - VIII. Properties of 1687 Gaia selected members in 21 nearby clusters
DOI: 10.1093/mnras/stae311 Bibcode: 2024MNRAS.529.1283F

Scholz, Aleks; Eislöffel, Jochen; Dvorak, Shawn +60 more

The Hunting Outbursting Young Stars (HOYS) project performs long-term, optical, multifilter, high cadence monitoring of 25 nearby young clusters and star-forming regions. Utilizing Gaia DR3 data, we have identified about 17 000 potential young stellar members in 45 coherent astrometric groups in these fields. Twenty one of them are clear young gro…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 3
Is It Possible to Detect Coronal Mass Ejections on Solar-type Stars through Extreme-ultraviolet Spectral Observations?
DOI: 10.3847/1538-4357/ad2a44 Bibcode: 2024ApJ...966...24Y

Tian, Hui; Yang, Zihao; Xu, Yu +3 more

Stellar coronal mass ejections (CMEs) from host stars are an important factor that affects the habitability of exoplanets. Although their solar counterparts have been well observed for decades, it is still very difficult to find solid evidence of stellar CMEs. Using the spectral line profile asymmetry caused by the Doppler shift of erupting plasma…

2024 The Astrophysical Journal
Hinode 3
Photometric determination of main-sequence binaries with Gaia
DOI: 10.1093/mnras/stad3789 Bibcode: 2024MNRAS.527.8718W

Wallace, A. L.

Since its launch in 2013, the Gaia space telescope has provided precise measurements of the positions and magnitudes of over 1 billion stars. This has enabled extensive searches for stellar and substellar companions through astrometric and radial velocity measurements. However, these surveys require a prior knowledge of any unresolved companion af…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 3
AB Dor: Coronal Imaging and Activity Cycles
DOI: 10.3847/1538-4357/ad2f2e Bibcode: 2024ApJ...966...86S

Pandey, J. C.; Singh, Gurpreet

Using long-term X-ray observations, we present short-term and long-term X-ray variability analysis of the ultrafast rotating active star AB Dor. Flaring events are common in X-ray observations of AB Dor and occupy a substantial portion of the total observation time, averaging at around 57% ± 23%. The flare-free X-ray light curves show rotational m…

2024 The Astrophysical Journal
Exosat XMM-Newton 3
First High-resolution Spectroscopy of X-Ray Absorption Lines in the Obscured State of NGC 5548
DOI: 10.3847/1538-4357/ad1bcb Bibcode: 2024ApJ...962..155M

Gu, Liyi; Kriss, Gerard A.; Mehdipour, Missagh +5 more

Multiwavelength spectroscopy of NGC 5548 revealed remarkable changes due to the presence of an obscuring wind from the accretion disk. This broadened our understanding of obscuration and outflows in active galactic nuclei. Swift monitoring of NGC 5548 shows that over the last 10 yr, the obscuration has gradually declined. This provides a valuable …

2024 The Astrophysical Journal
eHST 3
An Infrared Census of R Coronae Borealis Stars II—Spectroscopic Classifications and Implications for the Rate of Low-mass White Dwarf Mergers
DOI: 10.1088/1538-3873/ad6210 Bibcode: 2024PASP..136h4201K

Soria, Roberto; Clayton, Geoffrey C.; De, Kishalay +18 more

We present results from a systematic infrared (IR) census of R Coronae Borealis (RCB) stars in the Milky Way, using data from the Palomar Gattini IR (PGIR) survey. RCB stars are dusty, erratic variable stars presumably formed from the merger of a He-core and a CO-core white dwarf (WD). PGIR is a 30 cm J-band telescope with a 25 deg2 cam…

2024 Publications of the Astronomical Society of the Pacific
Gaia 3