|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
1999ApJS..124..181W - Astrophys. J., Suppl. Ser., 124, 181-193 (1999/September-0)
The interstellar environment of filled-center supernova remnants. III. The Crab nebula.
WALLACE B.J., LANDECKER T.L., KALBERLA P.M.W. and TAYLOR A.R.
Abstract (from CDS):
The H I environment of the Crab Nebula is investigated using 2'.75 and 9' resolution data from the Dominion Radio Astrophysical Observatory Synthesis and Effelsberg 100 m Radio Telescopes, respectively. No clear evidence for an interaction between the Crab and the surrounding H I is found; the Crab probably lies within the boundaries of a large-scale, low-density void in the H I distribution. The presence of a wind-blown H I bubble near the Crab is confirmed, and it is suggested that the unidentified star that powers this bubble is responsible for the stellar wind material detected along the line of sight toward the Crab.
Abstract Copyright: ∼
Journal keyword(s): ISM: Bubbles - ISM: General - ISM: Individual: Name: Crab Nebula - radio lines: ISM - supernova remnants
CDS comments: T.3: Bubble N = [WLT94] Bubble N.
Simbad objects: 7
To bookmark this query, right click on this link: simbad:1999ApJS..124..181W and select 'bookmark this link' or equivalent in the popup menu