M. Vučković
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View article: Dataset from the paper: "RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich"
Dataset from the paper: "RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich" Open
The two files contain the Tables presented in Appendix B of Bobrick & Iorio et al. (2024, MNRAS, 527, 12196–12218)(https://ui.adsabs.harvard.edu/abs/2024MNRAS.52712196B/abstract) in CSV format. # V3 updates - New columns added: GRRL, Gcomp…
View article: A comprehensive search for hot subdwarf stars using <i>Gaia</i> and TESS
A comprehensive search for hot subdwarf stars using <i>Gaia</i> and TESS Open
Context . Hot subdwarfs are compact, evolved stars that serve as critical testbeds for understanding binary evolution, stellar remnants, and pulsation physics. Their formation is often attributed to binary interactions, but a significant f…
View article: Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars
Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars Open
Context. Binary hot subdwarf B (sdB) stars are typically produced from low-mass red giant branch (RGB) stars that have lost almost all their envelopes through binary mass transfer while still fusing helium in their cores. Particularly, whe…
View article: Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars II. Sample validation
Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars II. Sample validation Open
We investigate the progenitors of long-period hot subdwarf B (sdB) binaries, which form when low-mass red giant branch (RGB) stars lose their envelopes through stable Roche lobe overflow (RLOV) near the tip of the RGB. We aim to expand our…
View article: Searching for new variable white dwarfs: The discovery of the three new pulsating and three new binary systems
Searching for new variable white dwarfs: The discovery of the three new pulsating and three new binary systems Open
In recent years, approximately 150 low-mass white dwarfs (WDs), typically with masses below 0.4 M ⊙ , have been discovered. Observational evidence indicates that most of these low-mass WDs are in binary systems, supporting binary evolution…
View article: Searching for new variable white dwarfs: The discovery of the three new pulsating and three new binary systems
Searching for new variable white dwarfs: The discovery of the three new pulsating and three new binary systems Open
In recent years, approximately 150 low-mass white dwarfs (WDs), typically with masses below 0.4 solar masses, have been discovered. Observational evidence indicates that most of these low-mass WDs are found in binary systems, supporting bi…
View article: Early detection of osteoporosis in a general practitioner's office
Early detection of osteoporosis in a general practitioner's office Open
Introduction. Identifying certain risk factors for osteoporosis can greatly influence its occurrence, progression, and overall outcomes. Objective. Our research focused on osteoporosis and its risk factors in menopausal women attending a g…
View article: Early detection of osteoporosis in a general practitioner's office
Early detection of osteoporosis in a general practitioner's office Open
Introduction. Identifying certain risk factors for osteoporosis can greatly influence its occurrence, progression, and overall outcomes. Objective. Our research focused on osteoporosis and its risk factors in menopausal women attending a g…
View article: The BlackGEM Telescope Array. I. Overview
The BlackGEM Telescope Array. I. Overview Open
The main science aim of the BlackGEM array is to detect optical counterparts to gravitational wave mergers. Additionally, the array will perform a set of synoptic surveys to detect Local Universe transients and short timescale variability …
View article: A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties
A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties Open
We present the first volume-limited sample of spectroscopically confirmed hot subluminous stars out to 500 pc, defined using the accurate parallax measurements from the {\em Gaia} space mission data release 3 (DR3). The sample comprises a …
View article: A 500 pc volume-limited sample of hot subluminous stars
A 500 pc volume-limited sample of hot subluminous stars Open
We present the first volume-limited sample of spectroscopically confirmed hot subluminous stars out to 500 pc, defined using the accurate parallax measurements from the Gaia space mission data release 3 (DR3). The sample comprises a total …
View article: The double low-mass white dwarf eclipsing binary system J2102–4145 and its possible evolution
The double low-mass white dwarf eclipsing binary system J2102–4145 and its possible evolution Open
In recent years, about 150 low-mass white dwarfs (WDs), typically with masses below 0.4 M ⊙ , have been discovered. The majority of these low-mass WDs are observed in binary systems as they cannot be formed through single-star evolution wi…
View article: The double low-mass white dwarf eclipsing binary system J2102-4145 and its possible evolution
The double low-mass white dwarf eclipsing binary system J2102-4145 and its possible evolution Open
Approximately 150 low-mass white dwarfs, with masses below 0.4Msun, have been discovered. The majority of these low-mass WDs are observed in binary systems as they cannot be formed through single-star evolution within the Hubble time. In t…
View article: A comprehensive search for hot subdwarf stars using <i>Gaia</i> and TESS
A comprehensive search for hot subdwarf stars using <i>Gaia</i> and TESS Open
Hot subdwarf B (sdB) stars are evolved, subluminous, helium-burning stars that most likely form when red giant stars loose their hydrogen envelope via interactions with close companions. They play an important role in our understanding of …
View article: Hot subdwarf wind models with accurate abundances
Hot subdwarf wind models with accurate abundances Open
Context . Helium-dominated subdwarfs are core helium burning stars stripped of their envelope. The nuclear evolution of these stars alters surface abundances. Modified abundances impact the strength of the stellar wind. Aims . We aim to un…
View article: Hot subdwarf wind models with accurate abundances II. Helium-dominated merger products CD-46 8926 and CD-51 11879
Hot subdwarf wind models with accurate abundances II. Helium-dominated merger products CD-46 8926 and CD-51 11879 Open
We aim to understand the influence of evolutionary modified surface abundances on the strength of the stellar wind in the helium-dominated subdwarfs CD-46 8926 and CD-51 11879. We used our own optical spectroscopy combined with archival ul…
View article: And how are you?
And how are you? Open
Background: As GPs (general physicians) we are often quick to judge our patients on their diet, weight, and lifestyle. And we frequently offer advice on how they could change their bad habits but do we follow our own advice? Methods and Ob…
View article: RR Lyrae from binary evolution: abundant, young, and metal-rich
RR Lyrae from binary evolution: abundant, young, and metal-rich Open
RR Lyrae are a well-known class of pulsating horizontal branch stars widely used as tracers of old, metal-poor stellar populations. However, mounting observational evidence shows that a significant fraction of these stars may be young and …
View article: Current status of the Extension of the FRIPON network in Chile
Current status of the Extension of the FRIPON network in Chile Open
FRIPON is an efficient ground-based network for the detection and characterization of fireballs, which was initiated in France in 2016 with over one hundred cameras and which has been very successfully extended to Europe and Canada with on…
View article: The mass range of hot subdwarf B stars from MESA simulations
The mass range of hot subdwarf B stars from MESA simulations Open
Hot subdwarf B (sdB) stars are helium core burning stars that have lost almost their entire hydrogen envelope due to binary interaction. Their assumed canonical mass of ${M_{\mathrm{sdB}}}\sim 0.47$ M⊙ has recently been debated given a bro…
View article: The mass range of hot subdwarf B stars from MESA simulations
The mass range of hot subdwarf B stars from MESA simulations Open
Hot subdwarf B (sdB) stars are helium core burning stars that have lost almost their entire hydrogen envelope due to binary interaction. Their assumed canonical mass of $\rm M_{\mathrm{sdB}}\sim0.47 M_{\odot}$ has recently been debated giv…
View article: Dataset from the paper: "RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich"
Dataset from the paper: "RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich" Open
The two files contain the Tables in the Appendix of Bobrick&Iorio et al. 2023 (https://ui.adsabs.harvard.edu/abs/2022arXiv220804332B/abstract) in the csv format. The columns in the table are: - Age: age of the system since the zero-age mai…
View article: TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite
TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite Open
We present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have …
View article: Dataset from the paper: "RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich"
Dataset from the paper: "RR Lyrae From Binary Evolution: Abundant, Young and Metal-Rich" Open
The two files contain the Tables in the Appendix of Bobrick&Iorio et al. 2023 (https://ui.adsabs.harvard.edu/abs/2022arXiv220804332B/abstract) in the csv format. The columns in the table are: - Age: age of the system since the zero-age ma…
View article: Asteroseismology of hot subdwarf B stars observed with TESS: discovery of two new gravity mode pulsating stars
Asteroseismology of hot subdwarf B stars observed with TESS: discovery of two new gravity mode pulsating stars Open
TIC 033834484 and TIC 309658435 are long-period pulsating subdwarf B stars, which were observed extensively (675 and 621 days, respectively) by the Transiting Exoplanet Survey Satellite (TESS). The high-precision photometric light curve re…
View article: Asteroseismology of hot subdwarf B stars observed with TESS: discovery of two new gravity mode pulsating stars
Asteroseismology of hot subdwarf B stars observed with TESS: discovery of two new gravity mode pulsating stars Open
TIC033834484 and TIC309658435 are long-period pulsating subdwarf B star, which were observed extensively (675 and 621 days, respectively) by the Transiting Exoplanet Survey Satellite (TESS). The high-precision photometric light curve revea…
View article: Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars
Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars Open
Context. Current theory predicts that hot subdwarf binaries are produced from evolved low-mass binaries that have undergone mass transfer and drastic mass loss during either a common-envelope phase or a stable Roche-lobe overflow while on …
View article: Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars I. Sample selection and binary classification method
Volume-limited sample of low-mass red giant stars, the progenitors of hot subdwarf stars I. Sample selection and binary classification method Open
The current theory predicts that hot subdwarf binaries are produced from evolved low-mass binaries that have undergone mass transfer and drastic mass loss during either a common envelope phase or a stable Roche lobe overflow while on the r…
View article: Comparison between capacitive and resistive electronic transfer therapy and high-intensity laser therapy in pain conditions related to musculoskeletal disorders
Comparison between capacitive and resistive electronic transfer therapy and high-intensity laser therapy in pain conditions related to musculoskeletal disorders Open
Introduction: Musculoskeletal disorders (MSDs) imply damage to muscular or skeletal systems, which usually develop due to strenuous, repetitive activity, or an inflammation process. The therapy with capacitive and resistive electronic tran…