Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...283..117h&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 283, Aug. 1, 1984, p. 117-122.
Astronomy and Astrophysics
Astrophysics
73
Accretion Disks, Interstellar Gas, Molecular Clouds, Orion Nebula, Carbon, Line Spectra, Spatial Resolution, Spectrometers, Sulfur
Scientific paper
J = 1-0 emission of CS and C34S around Orion-KL has been mapped with an angular resolution of 33arcsec. The region of large CS integrated intensity has a single maximum near the KL nebula and is elongated NE-SW. The peak velocity shows a systematic shift along the axis of the elongated feature. This is consistent with an existence of a large rotating disk around the KL nebula. The disk is 4×104AU (0.2 pc) in diameter and is rotating with a period of 5×105yr×sin i, where i is the inclination.
Akabane Kenji
Chikada Yoshihiro
Hasegawa Takuya
Hirabayashi Hisahi
Inatani Junji
No associations
LandOfFree
CS around Orion-KL - A large rotating disk 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 CS around Orion-KL - A large rotating disk, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CS around Orion-KL - A large rotating disk will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1674208