Kinematics of ring-shaped nebulae in the LMC. I - The radial velocity field of N70

Details Kinematics of ring-shaped nebulae in the LMC. I - The radial velocity field of N70 Kinematics of ring-shaped nebulae in the LMC. I - The radial velocity field of N70

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....97..342r&link_type=abstract

Astronomy and Astrophysics, vol. 97, no. 2, Apr. 1981, p. 342-346. Research supported by the Consejo Nacional de Ciencia y Tecn

Astronomy and Astrophysics

Astrophysics

24

Kinematics, Magellanic Clouds, Nebulae, Radial Velocity, Astronomical Models, Ring Structures, Shock Wave Propagation, Supernova Remnants

Scientific paper

New kinematical data from the ring-shaped nebula N70 in the LMC shows an
expansion velocity of 70 km/s. These data, together with the known
spectroscopic information can be explained by a shock model. The shock
origins are investigated. They are not likely to proceed from stellar
winds and should be attributed to an old supernova explosion.

Affiliated with

Also associated with

No associations

Rating

Kinematics of ring-shaped nebulae in the LMC. I - The radial velocity field of N70 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Kinematics of ring-shaped nebulae in the LMC. I - The radial velocity field of N70, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinematics of ring-shaped nebulae in the LMC. I - The radial velocity field of N70 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-781139