ºÝºÝߣshows by User: TigranKhanzadyan / http://www.slideshare.net/images/logo.gif ºÝºÝߣshows by User: TigranKhanzadyan / Fri, 13 Feb 2015 06:05:14 GMT ºÝºÝߣShare feed for ºÝºÝߣshows by User: TigranKhanzadyan SED of IRS 3¨CIRS 7 /slideshow/sed-fits/44638128 sed-fits-150213060515-conversion-gate02
SED of IRS 3¨CIRS 7. Filled circles are the data points and the triangles are lower and upper limits where errors are generally smaller than the data points. The solid black line indicates the best-fitting model, and the grey lines show all models that also fit the data satisfying the ¦Ö2 ?¦Ö2 best < 3 per data point criteria. The dashed line shows the SED of the assumed stellar photosphere in the best-fitting model.]]>

SED of IRS 3¨CIRS 7. Filled circles are the data points and the triangles are lower and upper limits where errors are generally smaller than the data points. The solid black line indicates the best-fitting model, and the grey lines show all models that also fit the data satisfying the ¦Ö2 ?¦Ö2 best < 3 per data point criteria. The dashed line shows the SED of the assumed stellar photosphere in the best-fitting model.]]>
Fri, 13 Feb 2015 06:05:14 GMT /slideshow/sed-fits/44638128 TigranKhanzadyan@slideshare.net(TigranKhanzadyan) SED of IRS 3¨CIRS 7 TigranKhanzadyan SED of IRS 3¨CIRS 7. Filled circles are the data points and the triangles are lower and upper limits where errors are generally smaller than the data points. The solid black line indicates the best-fitting model, and the grey lines show all models that also fit the data satisfying the ¦Ö2 ?¦Ö2 best &lt; 3 per data point criteria. The dashed line shows the SED of the assumed stellar photosphere in the best-fitting model. <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/sed-fits-150213060515-conversion-gate02-thumbnail.jpg?width=120&amp;height=120&amp;fit=bounds" /><br> SED of IRS 3¨CIRS 7. Filled circles are the data points and the triangles are lower and upper limits where errors are generally smaller than the data points. The solid black line indicates the best-fitting model, and the grey lines show all models that also fit the data satisfying the ¦Ö2 ?¦Ö2 best &amp;lt; 3 per data point criteria. The dashed line shows the SED of the assumed stellar photosphere in the best-fitting model.
SED of IRS 3¸MµÄRS 7 from Tigran Khanzadyan
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Area containing MHO735, 736 and 737 /slideshow/irs3and6/44638118 irs3and6-150213060509-conversion-gate01
Area containing MHO735, 736 and 737. Positions of IRS objects are shown by the crosses in both panels. Dotted arrows in the panels show the possible outflow direction. Panel (a) shows the H2 1¨C0 S(1) emission. Panel (b) is a colour-composite image constructed from 3.6¦Ìm (blue), 4.5¦Ìm (green) and 8.0¦Ìm (red) Spitzer IRAC bands where the position of MHO735 is shown by a filled circle for an easy comparison and a dotted bow-shock outlines the position of MHO737.]]>

Area containing MHO735, 736 and 737. Positions of IRS objects are shown by the crosses in both panels. Dotted arrows in the panels show the possible outflow direction. Panel (a) shows the H2 1¨C0 S(1) emission. Panel (b) is a colour-composite image constructed from 3.6¦Ìm (blue), 4.5¦Ìm (green) and 8.0¦Ìm (red) Spitzer IRAC bands where the position of MHO735 is shown by a filled circle for an easy comparison and a dotted bow-shock outlines the position of MHO737.]]>
Fri, 13 Feb 2015 06:05:09 GMT /slideshow/irs3and6/44638118 TigranKhanzadyan@slideshare.net(TigranKhanzadyan) Area containing MHO735, 736 and 737 TigranKhanzadyan Area containing MHO735, 736 and 737. Positions of IRS objects are shown by the crosses in both panels. Dotted arrows in the panels show the possible outflow direction. Panel (a) shows the H2 1¨C0 S(1) emission. Panel (b) is a colour-composite image constructed from 3.6¦Ìm (blue), 4.5¦Ìm (green) and 8.0¦Ìm (red) Spitzer IRAC bands where the position of MHO735 is shown by a filled circle for an easy comparison and a dotted bow-shock outlines the position of MHO737. <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/irs3and6-150213060509-conversion-gate01-thumbnail.jpg?width=120&amp;height=120&amp;fit=bounds" /><br> Area containing MHO735, 736 and 737. Positions of IRS objects are shown by the crosses in both panels. Dotted arrows in the panels show the possible outflow direction. Panel (a) shows the H2 1¨C0 S(1) emission. Panel (b) is a colour-composite image constructed from 3.6¦Ìm (blue), 4.5¦Ìm (green) and 8.0¦Ìm (red) Spitzer IRAC bands where the position of MHO735 is shown by a filled circle for an easy comparison and a dotted bow-shock outlines the position of MHO737.
Area containing MHO735, 736 and 737 from Tigran Khanzadyan
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Plants on Other Planets May Not be Green /TigranKhanzadyan/jt20070430 jt20070430-150213045834-conversion-gate01
"Plants on Other Planets May Not be Green" presentation was given during a Journal-Club meeting on 30th of April 2007 at National University of Ireland, Galway]]>

"Plants on Other Planets May Not be Green" presentation was given during a Journal-Club meeting on 30th of April 2007 at National University of Ireland, Galway]]>
Fri, 13 Feb 2015 04:58:34 GMT /TigranKhanzadyan/jt20070430 TigranKhanzadyan@slideshare.net(TigranKhanzadyan) Plants on Other Planets May Not be Green TigranKhanzadyan "Plants on Other Planets May Not be Green" presentation was given during a Journal-Club meeting on 30th of April 2007 at National University of Ireland, Galway <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/jt20070430-150213045834-conversion-gate01-thumbnail.jpg?width=120&amp;height=120&amp;fit=bounds" /><br> &quot;Plants on Other Planets May Not be Green&quot; presentation was given during a Journal-Club meeting on 30th of April 2007 at National University of Ireland, Galway
Plants on Other Planets May Not be Green from Tigran Khanzadyan
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Dissection of a Cold, Infalling High-Mass Star-Forming Core /TigranKhanzadyan/cork-asgi-talk cork-asgitalk-150213045344-conversion-gate02
"Dissection of a Cold, Infalling High-Mass Star-Forming Core" presentation was given during ASGI Autumn Meeting at UCC, 3rd of October 2008]]>

"Dissection of a Cold, Infalling High-Mass Star-Forming Core" presentation was given during ASGI Autumn Meeting at UCC, 3rd of October 2008]]>
Fri, 13 Feb 2015 04:53:44 GMT /TigranKhanzadyan/cork-asgi-talk TigranKhanzadyan@slideshare.net(TigranKhanzadyan) Dissection of a Cold, Infalling High-Mass Star-Forming Core TigranKhanzadyan "Dissection of a Cold, Infalling High-Mass Star-Forming Core" presentation was given during ASGI Autumn Meeting at UCC, 3rd of October 2008 <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/cork-asgitalk-150213045344-conversion-gate02-thumbnail.jpg?width=120&amp;height=120&amp;fit=bounds" /><br> &quot;Dissection of a Cold, Infalling High-Mass Star-Forming Core&quot; presentation was given during ASGI Autumn Meeting at UCC, 3rd of October 2008
Dissection of a Cold, Infalling High-Mass Star-Forming Core from Tigran Khanzadyan
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Looking at the Universe through Infrared Spectacles /slideshow/gac-talk090131/44634632 gac-talk090131-150213041809-conversion-gate02
"Looking at the Universe through Infrared Spectacles" is public out-reach lecture given on Galway Astronomy Festival 2009. It took place in Westwood House Hotel, January 30th 2009, Galway, Ireland]]>

"Looking at the Universe through Infrared Spectacles" is public out-reach lecture given on Galway Astronomy Festival 2009. It took place in Westwood House Hotel, January 30th 2009, Galway, Ireland]]>
Fri, 13 Feb 2015 04:18:09 GMT /slideshow/gac-talk090131/44634632 TigranKhanzadyan@slideshare.net(TigranKhanzadyan) Looking at the Universe through Infrared Spectacles TigranKhanzadyan "Looking at the Universe through Infrared Spectacles" is public out-reach lecture given on Galway Astronomy Festival 2009. It took place in Westwood House Hotel, January 30th 2009, Galway, Ireland <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/gac-talk090131-150213041809-conversion-gate02-thumbnail.jpg?width=120&amp;height=120&amp;fit=bounds" /><br> &quot;Looking at the Universe through Infrared Spectacles&quot; is public out-reach lecture given on Galway Astronomy Festival 2009. It took place in Westwood House Hotel, January 30th 2009, Galway, Ireland
Looking at the Universe through Infrared Spectacles from Tigran Khanzadyan
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https://cdn.slidesharecdn.com/profile-photo-TigranKhanzadyan-48x48.jpg?cb=1540379154 https://cdn.slidesharecdn.com/ss_thumbnails/sed-fits-150213060515-conversion-gate02-thumbnail.jpg?width=320&height=320&fit=bounds slideshow/sed-fits/44638128 SED of IRS 3¨CIRS 7 https://cdn.slidesharecdn.com/ss_thumbnails/irs3and6-150213060509-conversion-gate01-thumbnail.jpg?width=320&height=320&fit=bounds slideshow/irs3and6/44638118 Area containing MHO735... https://cdn.slidesharecdn.com/ss_thumbnails/jt20070430-150213045834-conversion-gate01-thumbnail.jpg?width=320&height=320&fit=bounds TigranKhanzadyan/jt20070430 Plants on Other Planet...