Featured Images

Images taken by Glenn Reagan, HOU TRA

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  M8
Tzecmaun BigMak image of M8 taken August 23, 2009. Red -Ha; Green - OIII; Blue - SII.
NGC 6992 (Network Nebla)
Part of the larger Veil Nebula in Cygnus, NGC 6992 is also known as the Network Nebula some 1400 light years distant. The Tzec Maun images were taken Aug.2, 2009. This BigMak image is H alpha (red), OIII(green), and SII(blue) composite.
NGC 6992 (Network Nebla)
Another image of NGC 6992 taken Aug.2, 2009. The AP206 image is RGB.
47 Tucanae (NGC 104)
47 Tucanae (NGC 104), globular cluster, about 16,700 light years away from Earth, and 120 light years across. Visible with the naked eye--the second brightest globular cluster in the sky (after Omega Centauri). Image by Glenn Reagan using the HOU Perth R-COP (Remote Telescope Partnership: Clarion University, Oil Region Astronomical Society, Perth Observatory) telescope.
30 Doradus
30 Doradus, originally thought to be a star, is the Tarantula nebula, an immense star forming region in The Large Magellanic Cloud. It is about 1,000 LY across, and 180,000 LY away. It is the most active starburst region known in the Local Group of galaxies. To give an idea of its size, if it were at the distance of the Orion Nebula (1,500 LY) from us, it would cover about 30 degrees (60 full moons) of the sky and would be so bright, it would cast shadows. It contains some of the most massive stars known and the closest supernova since the invention of the telescope, Supernova 1987A, occurred in the outskirts of this nebula.
Image by Glenn Reagan using the HOU Perth R-COP (Remote Telescope Partnership: Clarion University, Oil Region Astronomical Society, Perth Observatory) telescope.
M8
Tzecmaun BigMak image of M8 taken August 23 2009. Red -Ha; Green - OIII; Blue - SII.
NGC 6992
This 3-color RGB image was taken with the Tzec Maun Takahashi FSQ-106 apo refractor telescope using a SBIG STL 11000M CCD imager. With an f/5 focal ratio this telescope is great for larger images. Again NGC 6992 is the north eastern part of the Veil SNR complex. It's a great image for the beginner. My exposure times for RGB were 7,8,8 min. Could easily go with 10,10,10 min because the scope has an autoguider feature. Taken Aug 15, 2009.
NGC 6992 (Network Nebla)
Part of the larger Veil Nebula in Cygnus, NGC 6992 is also known as the Network Nebula some 1400 light years distant. The Tzec Maun images were taken Aug.2, 2009. This BigMak image is H alpha (red), OIII(green), and SII(blue) composite.

Another image of NGC 6992 taken Aug.2, 2009. The AP206 image is RGB.
M8
Image of M8 taken with Tzec Maun 14" BigMak reflecting telescope using narrow band H alpha (red), Oxygen III (green), and Sulfur II (blue) filters.
NGC5139 20090422.ngc5139.RCOP
2009-04-22 ngc5139 RCOP Glenn Reagan
M17 20090422.m17.RCOP
2009-04-22 m17 RCOP Glenn Reagan

Narrow band composite image of M42.
H alpha-Red, OIII-Green, SII-Blue.
Taken remotely 2009-03-19,
Tzec Maun Observatory-New Mexico.
IC443 H-S-O-Hi 20090103 Reagan
IC443 H-S-O-Hi 2009-01-03 Glenn Reagan
2090123 NGC2070
2009-01-23 NGC2070 rgb RCOP2 Glenn Reagan
M1
Horsehead Nebula

Two views of M8 - Lagoon Nebula taken June 26, 2009, by Glenn Reagan at the Hands-On Universe conference at Yerkes Observatory, Williams Bay WI, acquired remotely using the AP 206 Refractor at Tzec Maun Observatory in New Mexico. This image taken with H-alpha filter. Glenn Reagan is HOU TRA, Astronomy-Physics Teacher at Cordova High School, District Curriculum Lead Secondary Science Teacher, and professor at Folsom Lake College - El Dorado Center - Sacramento City College.  
M8 - Lagoon Nebula taken June 26, 2009, by Glenn Reagan at the Hands-On Universe conference at Yerkes Observatory, Williams Bay WI, acquired remotely using the AP 206 Refractor at Tzec Maun Observatory in New Mexico. This image is a color composite made from 3 separate images with color filters.
eta carina
A 3 color composite image of the Eta Carinae nebula (NGC 3372, the Keyhole Nebula) in the southern hemisphere some 7000-9000 LY distant. Image by Glenn Reagan, HOU TRA-Teacher - Cordova High School Folsom Lake College - El Dorado Center - Sacramento City College, using the Tzec Maun Australian telescope, a Takahashi TOA-150 (6") refractor, with a SBIG STL-11000 CCD and filter wheel. Operating the telescope remotely over the Internet, Glen took the images Friday March 1 in Pingelly, Australia (western Australia near Perth). Exposure times (RGB) were 3 min, 3 min, and 5 min. The image was processed with Photoshop CS2 using the ESA FITS Liberator plug-in.  
M8
July 2008. Color image of M8 by HOU TRA Glenn Reagan (Astronomy-Physics Teacher - Cordova High School Folsom Lake College - El Dorado Center - Sacramento City College). Camera AP206 was able to resolve the turbulent cloud structure around this star formation region. Telescope: 8" refractor. 3-color composite made using SalsaJ.
M3 is a globular cluster. It is composed of about a million older stars that formed near the birth of our galaxy, while the galaxy was still in a spherical shape. Image taken with the 0.9 meter (36") telescope at the NOAO Kitt Peak National Observatory in southern Arizona during the last week in June 2005 by teacher teams who were a part of the TLRBSE program offered by NOAO. -HOU TRA Glenn Reagan   M16 (the Eagle Nebula) is imaged in clear and H alpha filters. It is a molecular gas cloud region in which new stars are forming. Image taken with the 0.9 meter (36") telescope at the NOAO Kitt Peak National Observatory in southern Arizona during the last week in June 2005 by teacher teams who were a part of the TLRBSE program offered by NOAO. -HOU TRA Glenn Reagan
From HOU TRA Glenn Reagan: Thought you would enjoy this 3 color (RGB) composite
image I took last Saturday (12 Nov 2006) morning with the AP 206 telescope of Tzec Maun Observatory in New Mexico. The Tzec Maun Foundation is seeking teachers who would
like for their students to take images of various astronomical objects (www.tzec-maun.com).
  M51 (the Whirlpool Galaxy) was taken on June 30, just 2 days after a supernova was discovered in it. The SN light was still increasing in brightness at this time. (The SN is the bright star just below the lower galaxy's bright core in the first spiral arm.) Image taken with the 0.9 meter (36") telescope at the NOAO Kitt Peak National Observatory in southern Arizona during the last week in June 2005 by teacher teams who were a part of the TLRBSE program offered by NOAO. -HOU TRA Glenn Reagan

M51

Supernova 2005CS
...More on this supernova

Thu, 30 Jun 2005 M 51 Supernova (three color composite) Taken during NOAO's TLRBSE program, Kitt Peak. SN is tiny yellow dot just above the galactic core in the first spiral arm. Submitted by HOU TRA Glenn Reagan, Astronomy-Physics Teacher, Cordova High School Folsom Lake College - El Dorado Center, Sacramento City College

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M42 Image by Glenn Reagan
From HOU TRA Glenn Reagan:
image of M42 taken 12 Nov 2005 with the AP 206 telescope of Tzec Maun Observatory in New Mexico. (http://www.tzec-maun.com)

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Lawrence Hall of Science | © Tuesday, 24-Nov-2009 12:13:17 PST Regents of the University of California | Updated Wednesday, 28-Oct-2009 11:51:57 PDT