Showing posts with label WIYN. Show all posts
Showing posts with label WIYN. Show all posts

Thursday, December 20, 2012

Astro-Photography: Cygnus Loop Filaments

As an end of the year finale, the National Optical Astronomy Observatory (NOAO) and WIYN partners offer this new wide-field image of the Cygnus loop.

The Cygnus Loop is a large supernova remnant: the gaseous remains of a massive star that exploded long ago.

It is located about 1,500 light-years from Earth in the direction of the constellation Cygnus, the Swan.

Astronomers estimate the supernova explosion that produced the nebula occurred between 5,000 to 10,000 years ago.

First noted in 1784 by William Herschel, it is so large that its many parts have been catalogued as separate objects, including NGC 6992, NGC 6995 and IC 1340 along the eastern (left) side of the image, NGC 6974 and NGC 6979 near the top-center, and the Veil Nebula (NGC 6960) and Pickering’s Triangle along the western (right) edge.

The bright star near the western edge of the image, known as 52 Cygnus, is not associated with the supernova.

The data were obtained with the NOAO Mosaic 1 camera, with observations in the Oxygen [OIII] (blue), Sulphur [S II] (green) and Hydrogen-Alpha (red) filters. 

Sunday, December 9, 2012

One Degree Imager (ODI): The Bubble Nebula Observed

The Bubble Nebula (NGC 7635) captured by the new One Degree Imager (ODI) camera on WIYN. 

This wide field view, showing the nebulosity carved out by the winds of the massive central star, demonstrates the exquisite image quality.

An image of the central portion of the nebula, cosmetically corrected, is found here.

Image Credit: T.A. Rector (University of Alaska Anchorage), WIYN ODI team and WIYN/NOAO/AURA/NSF.

Just in time for the holidays, a spectacular image of the Bubble Nebula (NGC 7635) demonstrates the potential of the new camera known as the One Degree Imager, or ODI, that is being commissioned at the WIYN 3.5-meter telescope on Kitt Peak.

The Bubble Nebula is a shell of gas and dust carved out by the stellar wind of the massive central star (BD+60 2522), and ionized by the same star's high-energy light.

Located in the constellation Cassiopeia, this nebula is about 10 light-years across.

The accompanying wide field of the Bubble Nebula covers an area of the sky of 25 by 25 arc minutes, just a little smaller than the full moon.

The exquisite resolution, or sharpness, of the stars right to the edge of the image is a hint of things to come.

This image of the Bubble Nebula was created using three different filters (referred to as g, r and i) which are then assigned to the colours blue, red and yellow, respectively.

The wide field colour image has not been fully corrected to remove all defects and artifacts from the data reduction process, but the accompanying smaller image showing the heart of the nebula is in a final form.

Colour combining of astronomical images is an art as well as a science: the work on this image was completed by Dr. Travis Rector, who explained, "When making an image in effect we are translating what the telescope can see into something our eyes can see.

In the process of generating an image we assign different colours to each filter that we use.

Where possible we assign colours to each filter that roughly correspond to what the human eye would see." More information on how these images are created is available here.

Even prior to colour combining, the data reduction process is a very complex multistage operation: the data from ODI are first processed by the Science Data Management group at the National Optical Astronomy Observatory (NOAO), then moved and archived at Indiana University's Pervasive Technology Institute, utilizing an NSF supercomputing facility.

Among the issues that must be addressed is simply the sheer number of pixels in the multiple CCDs. Currently, the camera is only operating with 13 of its eventual 64 CCDs.

When fully operational, the ODI camera will be able to image an area of the sky five times that of the full moon - far larger than any previous camera at the WIYN telescope.

Sensitive to visible light, the camera will be able to resolve objects to better than 0.4 arc seconds. More details about the ODI camera are available in a previous press release.