most citedTaking the pulse of the shortest orbital period binary system RX J0806.3+1527

3 citations · 3 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

5 papers · 1 filter

astro-ph2004

Extracting stellar parameters from observed spectra: the role of cross-correlation and minimum distance methods

Tomaz Zwitter, Ulisse Munari, Arnaud Siebert

One may consider cross-correlation routines applied to stellar spectra as a way to determine not only the radial velocities but also to assess the properties of stellar atmospheres…

astro-ph2004

Asiago eclipsing binaries program. II. V570 Per

P. M. Marrese, U. Munari, R. Sordo +3

The orbit and physical parameters of the double-lined eclipsing binary V570 Per, discovered by the Hipparcos satellite, are derived with formal errors better than 1% using high res…

astro-ph20043 cited

Taking the pulse of the shortest orbital period binary system RX J0806.3+1527

G. L. Israel, S. Covino, S. Dall'Osso +8

RX J0806.3+1527 is thought to be a 321s orbital period (the shortest known) double white dwarf binary system. According to the double degenerate binary (DDB) scenario this source i…

astro-ph2004

SB2 and eclipsing binaries with GAIA and RAVE

U. Munari, T. Zwitter, E. F. Milone

The expected performance of GAIA satellite on eclipsing binaries is reviewed on the basis of (a) combined Hipparcos and ground-based observations mimicking GAIA data harvest, and (…

astro-ph2003

Spectroscopy, Photometry and Micro-arcsec Astrometry of Binaries with the GAIA Space Mission and with the RAVE Experiment

Tomaz Zwitter, Ulisse Munari

GAIA astrometric mission of ESA will be very efficient in discovering binary and multiple stars with any orbital period, from minutes to millions of years. Main parameters of the r…