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Related papers: Exocomet signatures around the A-shell star $\Phi$…

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We present the results of exploratory HST observations to detect the emission lines of ions in the Beta Pic disk with the spectrograph slit placed off the star. Possible emission lines from FeII have been detected at $\sim 10^{-14}$erg cm-2…

This paper is framed within a large project devoted to studying the presence of circumstellar material around main sequence stars, and looking for exocometary events. The work concentrates on HR 10 (A2 IV/V), known for its conspicuous…

We combine nulling interferometry at 10 {\mu}m using the MMT and Keck Telescopes with spectroscopy, imaging, and photometry from 3 to 100 {\mu}m using Spitzer to study the debris disk around {\beta} Leo over a broad range of spatial scales,…

The source HD172555 is a young A7V star surrounded by a debris disk with a gaseous component. Here, we present the detection of variable absorption features detected simultaneously in the Ca II K and H doublet lines (at 3,933 and 3,968…

We present high resolution spectroscopy of the common proper motion system FH Leo (components HD 96273 and BD+07 2411B), which has been classified as a novalike variable due to an outburst observed by Hipparcos, and we present and review…

Astrophysics · Physics 2009-11-11 T. H. Dall , L. Schmidtobreick , N. C. Santos , G. Israelian

As a part of an on-going program to explore the signature of p-modes in solar-like stars by means of high-resolution absorption lines pectroscopy, we have studied four stars (alfaCMi, etaCas A, zetaHer A and betaVir). We present here new…

Astrophysics · Physics 2009-11-10 M. Martic , J. -C. Lebrun , T. Appourchaux , S. G. Korzennik

We analyze interstellar absorption features in the full UV spectrum of the nearby (d = 24 pc) B8 IVn star alpha Leo (Regulus) obtained at high resolution and high S/N by the HST ASTRAL Treasury program. We derive column densities for many…

Astrophysics of Galaxies · Physics 2017-02-01 Cecile Gry , Edward B. Jenkins

The nature of the tenuous disks around A stars has raised considerable controversy in the literature during the past decade. The debate whether or not the disk around beta Pictoris contains gaseous molecular hydrogen is only the most recent…

Astrophysics · Physics 2009-11-07 Inga Kamp , Gerd-Jan van Zadelhoff , Ewine van Dishoeck , Ronald Stark

Spectroscopic and photometric variability is widespread among O-type supergiants. It is linked to various phenomena affecting the star and its circumstellar environment, thereby providing direct information concerning them. To investigate…

Solar and Stellar Astrophysics · Physics 2025-08-05 Gregor Rauw , Yaël Nazé , Charles-Antoine Gilon

HST/STIS spectra of the small clumps and filaments closest to the central star in VY CMa reveal that the very strong K I emission and TiO and VO molecular emission, long thought to form in a dusty circumstellar shell, actually originate in…

The young (50-400 Myr) A3V star $\beta$ Leo is a primary target to study the formation history and evolution of extrasolar planetary systems as one of the few stars with known hot ($\sim$1600$^\circ$K), warm ($\sim$600$^\circ$K), and cold…

This paper reports the results of a near infrared spectroscopic survey of LINER galaxies undertaken with a new infrared spectrograph at the 5 m Hale telescope. The galaxy sample includes 11 LINERs with spectra covering the [FeII] (1.2567…

Astrophysics · Physics 2009-10-30 J. E. Larkin , L. Armus , R. A. Knop , B. T. Soifer , K. Matthews

Spectroscopy across spatially resolved stellar surfaces reveals spectral line profiles free from rotational broadening, whose gradual changes from disk center toward the stellar limb reflect an atmospheric fine structure that is possible to…

Solar and Stellar Astrophysics · Physics 2018-09-05 Dainis Dravins , Martin Gustavsson , Hans-Günter Ludwig

Context. The post-main-sequence evolution of massive stars remains poorly understood, particularly for blue supergiants. These objects play a crucial role in the dynamical and chemical evolution of galaxies and exhibit pronounced…

AD Leo (GJ 388) is an active dM3 flare star extensively observed both in the quiescent and flaring states. Since this active star is near the fully-convective boundary, to study in detail its long-term chromospheric activity could be an…

Solar and Stellar Astrophysics · Physics 2015-06-18 Andrea P. Buccino , Romina Petrucci , Emiliano Jofré , Pablo J. D. Mauas

HD 189733 is an exoplanetary system consisting of a transiting hot Jupiter and an active K2V-type main sequence star. We aim to use VLT/UVES high resolution echelle spectra to study a stellar flare. We have performed simultaneous analyses…

Solar and Stellar Astrophysics · Physics 2017-11-15 T. Klocova , S. Czesla , S. Khalafinejad , U. Wolter , J. H. M. M. Schmitt

Beta Pictoris is an A-type star hosting a complex planetary system with two massive gas giants and a prominent debris disk. Variable absorption lines in its stellar spectrum have been interpreted as signatures of exocomets (comet-like…

Solar and Stellar Astrophysics · Physics 2026-01-14 Jose Luis Gragera-Más , Santiago Torres , Alexander James Mustill , Eva Villaver

Debris disks are extrasolar analogs to our own Kuiper Belt and they are detected around at least 17% of nearby Sun-like stars. The morphology and dynamics of a disk encode information about its history, as well as that of any exoplanets…

We present the first observations of extragalactic pulsating stars in the K2 ecliptic survey of the Kepler space telescope. Variability of all three RR Lyrae stars in the dwarf spheroidal galaxy Leo IV were successfully detected, at a…

Solar and Stellar Astrophysics · Physics 2015-10-14 L. Molnár , A. Pál , E. Plachy , V. Ripepi , M. I. Moretti , R. Szabó , L. L. Kiss