Published June 1988 | Version v1
Report

The Progenitor of SN 1987A

Creators

  • 1. National Aeronautics and Space Administration, Greenbelt, MD (USA). Goddard Space Flight Center

Description

Spatially resolved IUE spectra (1150 - 2000 A) taken at the position of SN 1987A in March 1987 show that the 12th mag B3 I star Sk -690 202 has disappeared. Only the two fainter companion stars (Star 2 and Star 3) are now present near the site of the supernova. Sk -690 202 is the star which exploded to produce SN 1987A. The known characteristics of Sk -690 202 are consistent with the interpretation that the progenitor was a relatively compact star, having a high-velocity low-density stellar wind prior to the outburst. Recent IUE spectra of SN 1987 A (May 1988) show no evidence that Sk -690 202 still exists inside the expanding ejecta

Part of:
A decade of UV astronomy with the IUE satellite. Volume 1

Additional details

Publishing Information

Imprint Title
A decade of UV astronomy with the IUE satellite. Volume 1
Imprint Pagination
427 p.
Journal Page Range
p. 107-110.
Report number
ESA-SP--281

Conference

Title
Celebratory symposium on a decade of UV astronomy with the IUE satellite.
Dates
12-15 Apr 1988.
Place
Greenbelt, MD (USA).

INIS

Country of Publication
France
Country of Input or Organization
France
INIS RN
20058577
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
SUPERNOVAE; ULTRAVIOLET SPECTRA
Descriptors DEC
BINARY STARS; ERUPTIVE VARIABLE STARS; SPECTRA; STARS; VARIABLE STARS

Optional Information