SiO masers in R Aquarii and other infrared stars

Details SiO masers in R Aquarii and other infrared stars SiO masers in R Aquarii and other infrared stars

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...230..442z&link_type=abstract

Astrophysical Journal, Part 1, vol. 230, June 1, 1979, p. 442-448.

Other

42

Binary Stars, Infrared Stars, Masers, Silicon Oxides, Giant Stars, Late Stars, M Stars, Stellar Spectra

Scientific paper

Observations carried out with the Kitt Peak radio telescope have revealed SiO maser emission from R Aqr and eight other objects from the IRC catalog. Variations in the radial velocity of the R Aqr maser (v = 1, J = 2 to 1) may be used to establish the binary nature of this star within about 10 years. A measurement of the orbital period would indicate whether R Aqr is a close, contact or common envelope system. SiO maser radiation is detectable over a continuous radial velocity range of about 50 km/sec toward the Kleinmann-Low nebula; the 1(01) to 1(10) transition of CH3NCH2 was not observed.

Affiliated with

Also associated with

No associations

Rating

SiO masers in R Aquarii and other infrared stars 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 SiO masers in R Aquarii and other infrared stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SiO masers in R Aquarii and other infrared stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1775605