Zobrazeno 1 - 10
of 166
pro vyhledávání: '"I. J. Danziger"'
Autor:
M. Fraser, K. Takáts, A. Pastorello, S. J. Smartt, S. Mattila, M-T. Botticella, S. Valenti, M. Ergon, J. Sollerman, I. Arcavi, S. Benetti, F. Bufano, R. M. Crockett, I. J. Danziger, A. Gal-Yam, J. R. Maund, S. Taubenberger, M. Turatto
Publikováno v:
The Astrophysical Journal. 714:L280-L284
We report the identification of a source coincident with SN 2009kr in HST pre-explosion images. The object appears to be a single point source with an intrinsic colour V-I = 1.1 and M_V = -7.6. If this is a single star it would be a yellow supergiant
Autor:
Srdjan Samurovic, I. J. Danziger
Publikováno v:
Astronomy & Astrophysics. 458:79-88
Context. Of the various observational methods used to address the question of dark matter in early-type galaxies there is the possibility of spatial overlap in using kinematics of stars, clusters and X-ray halos. Aims. To investigate methods for the
Autor:
I. J. Danziger, S. A. Korotkiy, D. Yu. Tsvetkov, A. Elmhamdi, A. Volnova, M. V. Ereshko, A. P. Shulga
Publikováno v:
Astronomy & Astrophysics. 460:769-776
Aims: To derive observational properties and physical parameters of the progenitor stars of type IIP supernovae SN 2005ay and SN 2005cs from their U,B,V,R,I CCD photometry, and to define their velocity behaviour. Methods: Light curves are analysed, a
Publikováno v:
Astronomy & Astrophysics. 450:305-330
The spectroscopic properties of a selected optical photospheric spectra of core collapse supernovae (CCSNe) are investigated.Special attention is devoted to traces of hydrogen at early phases. The generated spectra are found to match the observed one
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 364:L33-L37
The progenitor of SN 2005cs, in the galaxy M51, is identified in pre-explosion HST ACS WFC imaging. Differential astrometry, with post-explosion ACS HRC F555W images, permitted the identification of the progenitor with an accuracy of 0.006". The prog
Autor:
Massimo Turatto, M. Della Valle, Enrico Cappellaro, Mark M. Phillips, A. Elmhamdi, C. Gouiffes, I. J. Danziger
Publikováno v:
Astronomy & Astrophysics. 426:963-977
Photometry and spectra of the type Ib SN 1990I are presented and analysed, covering about 400 days of evolution. The presence of optical helium lines is shown. SN 1990I seems to show higher velocities compared to a sample of type Ib events. The nebul
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 353:953-979
[Abridged] Deep optical observations of the spectra of 12 Galactic planetary nebulae (PNe) and 3 Magellanic Cloud PNe were presented in Paper I by Tsamis et al. (2003b), who carried out an abundance analysis using the collisionally excited forbidden
Publikováno v:
Astronomy & Astrophysics. 422:563-572
We report the detection of a cool stellar component at the center of the planetary nebula (PN) Me 1-1 and present optical spectra of the system. From measurements of nebular emission lines, we have derived electron temperature, density and chemical c
Autor:
I. J. Danziger, N. N. Chugai
Publikováno v:
Astronomy Letters. 29:649-657
We model the interaction of the supernova SN 1995G with a dense circumstellar (CS) gas in a thin shell approximation. A model fit of the observed bolometric light curve combined with data on the supernova expansion velocity provides an estimate of th
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 345:186-220
We present spectrophotometry of 12 Galactic and 3 Magellanic Cloud planetary nebulae (PNe). Nine of the Galactic PNe were observed by scanning the slit across the PN. We use the fluxes of collisionally excited lines (CELs) to derive electron densitie