RCW 102
Coordinates: (331.9°, -1.0°)
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Avedisova lists the ionising stars as the O6 III giant CD -51 9977, the B 0.5 Ia supergiant CP -51 9180 and the B1 Iab supergiant CD -51 9950.
According to a 2005 paper, RCW 102 consists of two objects at different distances. RCW 102b appears to be ionised by the O6 III giant LS 3539 = CD -51 9977. The photometric distance to the star is 4800 parsecs. (Although, confusingly, the paper refers to a second photometric estimate for other nearby stars of 4200 parsecs.) In contrast, the kinematic distance to the gas appears to be significantly less, 3500 parsecs, suggesting significant velocity dispersion in the Scutum-Crux (Centaurus) arm.
RCW 102 appears in the direction of the OB association R103 along with the supernova remnant RCW 103 and the HII region RCW 106.
RCW 102 is visible (although faint) in hydrogen-alpha but seems invisible at infrared and radio frequencies. It appears near the centre of a large bubble-like structure visible in this Parkes radio image here and in this MSX infrared image here.
You can view a rare visual image of this little photographed nebula here.
According to a 2005 paper, RCW 102 consists of two objects at different distances. RCW 102b appears to be ionised by the O6 III giant LS 3539 = CD -51 9977. The photometric distance to the star is 4800 parsecs. (Although, confusingly, the paper refers to a second photometric estimate for other nearby stars of 4200 parsecs.) In contrast, the kinematic distance to the gas appears to be significantly less, 3500 parsecs, suggesting significant velocity dispersion in the Scutum-Crux (Centaurus) arm.
RCW 102 appears in the direction of the OB association R103 along with the supernova remnant RCW 103 and the HII region RCW 106.
RCW 102 is visible (although faint) in hydrogen-alpha but seems invisible at infrared and radio frequencies. It appears near the centre of a large bubble-like structure visible in this Parkes radio image here and in this MSX infrared image here.
You can view a rare visual image of this little photographed nebula here.
RCW 102 consists of two objects at different distances. RCW 102B appears to be ionised by the O6 III LS 3539. The photometric distance to the star is 4800 parsecs. In contrast, the kinematic distance to the gas appears to be significantly less, 3500 parsecs, suggesting significant velocity dispersion in the Scutum-Crux arm. [1]
Notes
1. ^ Russeil, D., Adami, C., Amram, P., et al. (2005). "A deep Hα survey of the Milky Way. VI. The l = 332° area", Astronomy and Astrophysics, Vol. 429, 497-507. [2005A&A...429..497R]
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Most of the sources used to create these nebula descriptions are listed in the
notes section for each description. In some cases,
for example the Avedisova, Humphreys and Reed catalogs, the source is used extensively and is not listed in the
individual nebula descriptions. See this catalog overview
for more information on the catalogs and the general sources used
to create these descriptions and this introduction to HII regions
on the general history of this area of astronomy.
This image was created using the POSS-II/UKSTU data of the Digitized Sky Survey and SuperCOSMOS using the process described here.
According to my correspondence with the Royal Observatory Edinburgh and the Space Telescope Science Institute, I am allowed to use the POSS-II/UKSTU data to create and display images for non-commercial purposes so long as I include this fine print for the SuperCOSMOS data:
Use of these images is courtesy of the UK Schmidt Telescope (copyright in which is owned by the Particle Physics and Astronomy Research Council of the UK and the Anglo-Australian Telescope Board) and the Southern Sky Survey as created by the SuperCOSMOS measuring machine and are reproduced here with permission from the Royal Observatory Edinburgh.
and this acknowledgement taken from the DSS site:
The Digitized Sky Surveys were produced at the Space Telescope Science Institute under U.S. Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions.
The Second Palomar Observatory Sky Survey (POSS-II) was made by the California Institute of Technology with funds from the National Science Foundation, the National Geographic Society, the Sloan Foundation, the Samuel Oschin Foundation, and the Eastman Kodak Corporation.
The UK Schmidt Telescope was operated by the Royal Observatory Edinburgh, with funding from the UK Science and Engineering Research Council (later the UK Particle Physics and Astronomy Research Council), until 1988 June, and thereafter by the Anglo-Australian Observatory. The blue plates of the southern Sky Atlas and its Equatorial Extension (together known as the SERC-J), as well as the Equatorial Red (ER), and the Second Epoch [red] Survey (SES) were all taken with the UK Schmidt.
The "Second Epoch Survey" of the southern sky was made by the Anglo-Australian Observatory (AAO) with the UK Schmidt Telescope. Plates from this survey have been digitized and compressed by the ST ScI. The digitized images are copyright ? 1993-5 by the Anglo-Australian Observatory Board, and are distributed herein by agreement.
The "Equatorial Red Atlas" of the southern sky was made with the UK Schmidt Telescope. Plates from this survey have been digitized and compressed by the ST ScI. The digitized images are copyright ? 1992-5, jointly by the UK SERC/PPARC (Particle Physics and Astronomy Research Council, formerly Science and Engineering Research Council) and the Anglo-Australian Telescope Board, and are distributed herein by agreement.
The compressed files of the "Palomar Observatory - Space Telescope Science Institute Digital Sky Survey" of the northern sky, based on scans of the Second Palomar Sky Survey are copyright ? 1993-1995 by the California Institute of Technology and are distributed herein by agreement. The compressed files of the "Palomar Observatory - Space Telescope Science Institute Digital Sky Survey" of the northern sky, based on scans of the Second Palomar Sky Survey are copyright ? 1993-1995 by the California Institute of Technology and are distributed herein by agreement.