134 citations
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- Fernando Cruz-Sáenz de Miera7
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- Konkoly ObservatoryHU74 papers
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- Astronomical Observatory of CapodimonteIT11 papers
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49 papers · 1 filter
PENELLOPE V. The magnetospheric structure and the accretion variability of the classical T Tauri star HM Lup
A. Armeni, B. Stelzer, R. A. B. Claes +9
HM Lup is a young M-type star that accretes material from a circumstellar disk through a magnetosphere. Our aim is to study the inner disk structure of HM Lup and to characterize i…
A trio of month long flares in the nova-like variable V704 And
Gabriella Zsidi, C. J. Nixon, T. Naylor +2
We present the discovery of an unusual set of flares in the nova-like variable V704 And. Using data from AAVSO, ASAS-SN, and ZTF, of the nova-like variable V704 And, we have discov…
A high HDO/HO ratio in the Class I protostar L1551 IRS5
Audrey Andreu, Audrey Coutens, Fernando Cruz-Sáenz de Miera +4
Water is a very abundant molecule in star-forming regions. Its deuterium fractionation is an important tool for understanding its formation and evolution during the star and planet…
Predicting light curves of RR Lyrae variables using artificial neural network based interpolation of a grid of pulsation models
Nitesh Kumar, Anupam Bhardwaj, Harinder P. Singh +4
We present a new technique to generate the light curves of RRab stars in different photometric bands ( and bands) using Artificial Neural Networks (ANN). A pre-computed grid…
A multiphase study of theoretical and observed light curves of classical Cepheids in the Magellanic Clouds
Kerdaris Kurbah, Sukanta Deb, Shashi M. Kanbur +5
We present an analysis of the theoretical and observed light curve parameters of the fundamental mode (FU) classical Cepheids in the Magellanic Clouds in - and - photometric…
Empirical Determination of the Lithium 6707.856 Å Wavelength in Young Stars
Justyn Campbell-White, Carlo F. Manara, Aurora Sicilia-Aguilar +20
Absorption features in stellar atmospheres are often used to calibrate photocentric velocities for kinematic analysis of further spectral lines. The Li feature at 6708 Å is…