SIO Maser Survey of the Galactic Disk IRAS Sources. III. -10°<l<15° and |b|<=3°, a Central Part of the Galaxy

Details SIO Maser Survey of the Galactic Disk IRAS Sources. III. -10°<l<15° and |b|<=3°, a Central Part of the Galaxy SIO Maser Survey of the Galactic Disk IRAS Sources. III. -10°<l<15° and |b|<=3°, a Central Part of the Galaxy

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apjs..130..351d&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 130, Issue 2, pp. 351-379.

Astronomy and Astrophysics

Astronomy

20

Stars: Circumstellar Matter, Galaxy: Kinematics And Dynamics, Masers, Radio Lines: Stars, Stars: Late-Type

Scientific paper

A survey has been made in the SiO J=1-0, v=1 and 2 transitions (~43 GHz) for the color-selected IRAS sources in the central region of the Galaxy, -10deg

Affiliated with

Also associated with

No associations

Rating

SIO Maser Survey of the Galactic Disk IRAS Sources. III. -10°<l<15° and |b|<=3°, a Central Part of the Galaxy 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 Maser Survey of the Galactic Disk IRAS Sources. III. -10°<l<15° and |b|<=3°, a Central Part of the Galaxy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SIO Maser Survey of the Galactic Disk IRAS Sources. III. -10°<l<15° and |b|<=3°, a Central Part of the Galaxy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1769125