Principal     Comenzar     To Survive in the Universe    
Inhabited Sky
    News@Sky     Astrofotografía     La Colección     Foro     Blog New!     FAQ     Prensa     Login  

HD 157663


Contenidos

Imágenes

Subir su imagen

DSS Images   Other Images


Artículos relacionados

Evidence for Asphericity in the Type IIN Supernova SN 1998S
We present optical spectropolarimetry obtained at the Keck II 10 mtelescope on 1998 March 7 UT along with total flux spectra spanning thefirst 494 days after discovery (1998 March 2 UT) of the peculiar TypeIIn supernova (SN) 1998S. The SN is found to exhibit a high degree oflinear polarization, implying significant asphericity for itscontinuum-scattering environment. Prior to the removal of interstellarpolarization, the polarization spectrum is characterized by a flatcontinuum (at p~2%) with distinct changes in polarization associatedwith both the broad (symmetric, half-width near zero intensity>~10,000 km s-1) and narrow (unresolved, full width athalf-maximum less than 300 km s-1) line emission seen in thetotal flux spectrum. When analyzed in terms of a polarized continuumwith unpolarized broad-line recombination emission, an intrinsiccontinuum polarization of p~3% results, suggesting a global asphericityof >~45% from the oblate, electron-scattering dominated models ofHöflich. The smooth, blue continuum evident at early times is shownto be inconsistent with a reddened, single-temperature blackbody,instead having a color temperature that increases with decreasingwavelength. Broad emission-line profiles with distinct blue and redpeaks are seen in the total flux spectra at later times, suggesting adisklike or ringlike morphology for the dense(ne~107 cm-3) circumstellar medium,generically similar to what is seen directly in SN 1987A, although muchdenser and closer to the progenitor in SN 1998S. Implications of thecircumstellar scattering environment on the spectropolarimetry arediscussed, as are the effects of uncertainty in the removal ofinterstellar polarization; the importance of obtaining multiplespectropolarimetric epochs in future studies to help better constrainthe interstellar polarization value is particularly stressed. Usinginformation derived from the spectropolarimetry and the total fluxspectra, an evolutionary scenario for SN 1998S and its progenitor arepresented.

Enviar un nuevo artículo


Enlaces relacionados

  • - No se han encontrado enlaces -
En viar un nuevo enlace


Miembro de los siguientes grupos:


Datos observacionales y astrométricos

Constelación:Dragón
Ascensión Recta:17h16m57.67s
Declinación:+74°08'48.4"
Magnitud Aparente:8.283
Distancia:274.725 parsecs
Movimiento Propio en Ascensión Recta:-8.7
Movimiento Propio en Declinación:33.4
B-T magnitude:9.603
V-T magnitude:8.392

Catálogos y designaciones:
Nombres Propios   (Edit)
HD 1989HD 157663
TYCHO-2 2000TYC 4427-430-1
USNO-A2.0USNO-A2 1575-03776358
HIPHIP 84538

→ Solicitar más catálogos y designaciones a VizieR