Pregled bibliografske jedinice broj: 161178
A Second Stellar Color Locus: a Bridge from White Dwarfs to M stars
A Second Stellar Color Locus: a Bridge from White Dwarfs to M stars // Spectroscopically and Spatially Resolving the Components of the Close Binary Stars / Hilditch, R. W. ; Hensberge, H. ; Pavlovski, K. (ur.).
San Francisco (CA): Astronomical Society of the Pacific (ASP), 2004. str. 396-298 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
CROSBI ID: 161178 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
A Second Stellar Color Locus: a Bridge from White Dwarfs to M stars
Autori
Smolčić, V. ; Ivezić, Z. ; Knapp, G. R. ; Lupton, R. H. ; Pavlovski, K. ; Ilijić, S. ; Schlegel, D. ; Smith, J. A. ; McGehee, P. M. ; Silvestri, N. M. ; Hawley, S. L. ; Rockosi, C. ; Gunn, J. E. ; Strauss, M. A.
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
Spectroscopically and Spatially Resolving the Components of the Close Binary Stars
/ Hilditch, R. W. ; Hensberge, H. ; Pavlovski, K. - San Francisco (CA) : Astronomical Society of the Pacific (ASP), 2004, 396-298
Skup
Workshop on Spectroscopically and Spatially Resolving the Components of the Close Binary Stars
Mjesto i datum
Dubrovnik, Hrvatska, 20.10.2003. - 24.10.2003
Vrsta sudjelovanja
Poster
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
Sloan Digital Sky Survey; white dwarfs; M dwarfs; close binaries
Sažetak
We report the discovery of a locus of stars in the SDSS $g-r$ vs. $u-g$ color-color diagram that connects the colors of white dwarfs and M dwarfs. While its contrast with respect to the main stellar locus is only $\sim$1:2300, this previously unrecognized feature includes 863 stars from SDSS Data Release 1. The position and shape of the feature is in good agreement with predictions of a simple binary star model that consists of a white dwarf and an M dwarf, with the components' luminosity ratio controlling the position along this binary system locus. SDSS DR1 spectra for 47 of these objects strongly support this model.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Ustanove:
Fakultet elektrotehnike i računarstva, Zagreb,
Prirodoslovno-matematički fakultet, Zagreb