Miroshnichenko, A. S., Chentsov, E. L., Klochkova, V. G., Zharikov, S. V., Grankin, K. N., Kusakin, A. V., ...
FS CMa type stars are a group of Galactic objects with the B[e] phenomenon. They exhibit strong emission-line spectra and infrared excesses, which are most likely due to recently formed circumstellar...
Multisite photometry of the pulsating Herbig Ae star V346 Ori (2009)
Bernabei, S., Ripepi, V., Ruoppo, A., Marconi, M., Rodriguez, E., ...
CONTEXT: The study of pulsation in Pre--Main--Sequence intermediate-mass stars represents an important tool for deriving information on fundamental stellar parameters and internal structure, as well...
The planet-hosting subdwarf B star V391 Pegasi is a hybrid pulsator (2009)
Lutz, R., Schuh, S., Silvotti, R., Bernabei, S., Dreizler, S., Stahn, T., ...
A noticeable fraction of subdwarf B stars shows either short-period (p-mode) or long-period (g-mode) luminosity variations, with two objects so far known to exhibit hybrid behaviour, i.e. showing...
The O-C diagram of the subdwarf B pulsating star HS2201+2610: detection of a giant planet? (2007)
Silvotti, R., Schuh, S., Janulis, R., Bernabei, S., Ostensen, R., ...
In this article we present the O-C diagram of the hot subdwarf B pulsating star HS2201+2610 after seven years of observations. A secular increase of the main pulsation period,...
Overview of the Alcator C-MOD research programme (2007)
Scott, S., Bader, A., Bakhtiari, M., Basse, N., Beck, W., Biewer, T., ...
Discovery of $\delta$ Scuti pulsation in the Herbig Ae star VV Ser (2006)
Ripepi, V., Bernabei, S., Marconi, M., Ruoppo, A., Palla, F., ...
A new observational study of the Herbig Ae star VV Ser has been performed in order to detect and accurately measure pulsation frequencies in the $\delta$ Scuti range. As it belongs to the continuous...
Effect of plasma shaping on performance in the National Spherical Torus Experiment (2006)
Choe, Wonho, Gates, D. A., Maingi, R., Menard, J., Kaye, S., Sabbagh, S. A., ...
The National Spherical Torus Experiment (NSTX) has explored the effects of shaping on plasma performance as determined by many diverse topics including the stability of global magnetohydrodynamic...
A multisite photometric campaign on the Pre-Main-Sequence delta Scuti pulsator IP Per (2005)
Ripepi, V., Bernabei, S., Marconi, M., Palla, F., Ferro, A. Arellano, Bonanno, A., ...
We present the results of a photometric multisite campaign on the $\delta$ Scuti Pre-Main-Sequence star IP Per. Nine telescopes have been involved in the observations, with a total of about 190 hours...
Recent results on Pre-main sequence delta Scuti stars (2005)
Ripepi, V., Marconi, M., Palla, F., Bernabei, S., Ruoppo, A., Cusano, F., ...
Intermediate mass Pre-main sequence stars (1.5 $M_{\odot}< M < 5M_{\odot}$) cross the instability strip on their way to the main sequence. They are therefore expected to be pulsating in a similar way...
Overview of the Alcator C-Mod Program (2005)
Greenwald,M., Andelin,D., Basse,N., Bernabei,S., Bonoli,P., Böse,B., ...
Overview of the Alcator C-Mod Program (2005)
Greenwald,M., Andelin,D., Basse,N., Bernabei,S., Bonoli,P., Böse,B., ...
Overview of the Alcator C-Mod Program (2005)
Greenwald, M., Andelin, D., Basse, N., Bernabei, S., Bonoli, P., Böse, B., ...
Overview of the Alcator C-Mod Program (2005)
Greenwald, M., Andelin, D., Basse, N., Bernabei, S., Bonoli, P., Böse, B., ...
Overview of the Alcator C-Mod program (2005)
Greenwald, M., Andelin, D., Basse, N., Bernabei, S., Bonoli, P., Bose, B., ...
Research on the Alcator C-Mod tokamak has emphasized RF heating, self-generated flows, momentum transport, scrape-off layer (SOL) turbulence and transport and the physics of transport barrier...
Multisite observations of the PMS delta Scuti star V351 Ori (2003)
Ripepi, V., Marconi, M., Bernabei, S., Palla, F., Pinheiro, F. J. G., Folha, D. F. M., ...
We present the results of multisite observations spanning two years on the pre--main-sequence (PMS) star V351 Ori. A total of around 180 hours of observations over 29 nights have been collected,...
RF heating and current drive on NSTX with high harmonic fast waves (2003)
Ryan,P. M., Rosenberg,A. L., Swain,D. W., Wilson,J. R., Batchelor,D. B., Bell,M. G., ...
NSTX is a small aspect ratio tokamak (R = 0.85 m, a = 0.65 m). The High Harmonic Fast Wave (HHFW) system is a 30 MHz, 12-element array capable of launching both symmetric and directional wave spectra...
RF heating and current drive on NSTX with high harmonic fast waves (2003)
Ryan, P. M., Rosenberg, A. L., Swain, D. W., Wilson, J. R., Batchelor, D. B., Bell, M. G., ...
NSTX is a small aspect ratio tokamak (R = 0.85 m, a = 0.65 m). The High Harmonic Fast Wave (HHFW) system is a 30 MHz, 12-element array capable of launching both symmetric and directional wave spectra...
Overview of JET results (2003)
Pamela, J., Solano, E. R., Adams, J. M., Agarici, G., Agarici, M., Akhter, H., ...
Scientific and technical activities on JET focus on the issues likely to affect the ITER design and operation. Our understanding of the ITER reference mode of operation, the ELMy H-mode, has...
Detection of delta Scuti-like pulsation in H254, a pre-main sequence F-type star in IC 348 (2002)
Ripepi, V., Palla, F., Marconi, M., Bernabei, S., Ferro, A. Arellano, Terranegra, L., ...
We present time series observations of intermediate mass PMS stars belonging to the young star cluster IC 348. The new data reveal that a young member of the cluster, H254, undergoes periodic light...
The X-ray transient XTE J1859+226 in Outburst & Quiescence (2002)
Zurita, C., Sanchez-Fernandez, C., Casares, J., Charles, P. A., Abbott, T. M., Hakala, P., ...
We present optical photometry and spectroscopy of the X-ray transient XTE J1859+226, obtained during outburst and its subsequent decay to quiescence. Both the X-ray and optical properties are very...
LHCD Coupling During H-Mode and ITB in JET Plasmas (2001)
Ridolfini, V.P., Podda, S., Mailloux, J., Sarazin, Y., Baranov, Y., Bernabei, S., ...
Unusually rapid variability of the GRB000301C optical afterglow (2000)
Masetti, N., Bartolini, C., Bernabei, S., Guarnieri, A., Palazzi, E., Pian, E., ...
We present BVRI light curves of the afterglow of GRB000301C, one of the brightest ever detected at a day time scale interval after GRB trigger. The monitoring started 1.5 days after the GRB and ended...