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• Studying Young Stars
  =Why should anyone care about young stars?= =Young stars in general: Introduction to (low-mass) star formation=
  13 KB (2,128 words) - 22:21, 23 March 2023
• Monitoring young stars
  ...fields of science, from tree rings to weather to sunspots to variations of young stars. There is a LOT of information out there on the web with information ...arch know that she is interested specifically in finding rotation rates in young stars. Finding periodic variations is a special case of finding variations
  5 KB (823 words) - 19:03, 13 May 2011
• General Background on young stars
  ...S more information on young stars in the [[Studying Young Stars | studying young stars]] section of the Advanced Research Tools. This page has a high-level
  3 KB (522 words) - 21:30, 11 December 2007

Page text matches

• Making Light Curves for our YSO Candidates
  ...toring young stars]], which is a general introduction to, well, monitoring young stars.
  2 KB (264 words) - 17:35, 21 December 2007
• Science background
  =Young Stars= *[[Studying Young Stars]] - More information on the study of young stars, by Dr. Luisa Rebull (2011)
  2 KB (366 words) - 17:02, 16 November 2020
• StarFormation
  ===Protostars vs Young Stars=== ...Many other, relatively short lived stars, E.g. O, B stars, are also called young stars.
  3 KB (395 words) - 23:10, 31 January 2013
• Info to help you answer questions and things I just don't get
  ...tary globules are Bok globules that have comet like tail (can contain many young stars BRCs (Bright Rimmed Clouds) are dense clumps of matter (can contain many young stars) in older HII regions which have been further compressed and illumina
  3 KB (413 words) - 02:40, 28 April 2012
• Taurus catalog
  ...stars, it is sometimes helpful to understand the color properties of other young stars. The Taurus Molecular Cloud (TMC) is one of the closest star forming ...oscopy, and in fact covers such a large region that some of the apparently young stars we found may in fact be members of adjacent star-forming regions (Ple
  4 KB (756 words) - 15:06, 11 May 2012
• General Background on young stars
  ...S more information on young stars in the [[Studying Young Stars | studying young stars]] section of the Advanced Research Tools. This page has a high-level
  3 KB (522 words) - 21:30, 11 December 2007
• Kitt Peak YSO Research Project
  T-Tauri stars are very young sun-like stars in the early stages of development, and are important to ast ...lowly forms into planetary objects or is blown off into space exposing the young star.
  5 KB (808 words) - 21:55, 23 October 2008
• BRC Bigger Picture and Goals
  ...her people did, and make sure that we are not, say, announcing "OMG 30 new young stars!!!1!" when in reality 25 of them were found before by someone else, a
  4 KB (711 words) - 03:00, 19 May 2011
• LW discussion of YSOs
  ===When is an object a young stellar object?=== Young Stellar Objects are stars in the earliest stage of development. Two Types:
  2 KB (369 words) - 21:24, 19 June 2012
• 2011 and earlier wiki team work
  ...is working with at least one bright-rimmed cloud (BRC) to characterize the young star population that might be found there. Much of the background informat ..., is working with multi-wavelength observations of CG4 to characterize the young star population that might be found there. Much of the background informat
  5 KB (772 words) - 17:09, 17 April 2013
• C-WAYS Bigger Picture and Goals
  We have WISE data for 3 patches of sky likely to harbor young stars: BRC 27, BRC 34, and BRC 38. ...her people did, and make sure that we are not, say, announcing "OMG 30 new young stars!!!1!" when in reality 25 of them were found before by someone else, a
  5 KB (824 words) - 23:33, 26 March 2012
• Color-color plot ideas
  * Young et al., 2004, ApJS, 154, 428, figures 3, 4, 5
  2 KB (280 words) - 23:54, 13 May 2008
• Wiki Development Plans
  **[[Monitoring young stars]] - very skeletal right now.
  1 KB (156 words) - 22:32, 7 October 2009
• Scary words
  ...nt out, this is not necessarily a good assumption for our specific case of young stars, as there are likely to be fluctuations intrinsic to the source that
  2 KB (230 words) - 21:49, 19 November 2007
• Current Research Projects
  This team, which started in Jan 2016, is looking for AGN in some surveys for young stars. ...d (Spitzer and WISE), optical (SDSS), and X-ray (Chandra) data to look for young stars in the Ceph C star-forming core.
  7 KB (1,059 words) - 22:10, 10 January 2017
• CG4 AAS 2011 Meeting
  ...1.JPG|500px|thumb|left|AAS Poster #248.13 Multi-Sensory Approach Finding Young Stellar Objects in CG4. People in picture are as follows. Back Row, left t ...0.JPG|400px|thumb|left|AAS Poster #248.13 Multi-Sensory Approach Finding Young Stellar Objects in CG4. People in picture are as follows. Back Row, left t
  2 KB (296 words) - 00:23, 19 January 2011
• Walter Payton College Prep High School
  == Cool, Wise and Young Stars Astronomy Research Group == [[Studying Young Stars]]
  6 KB (1,041 words) - 04:56, 22 June 2012
• Introduction to IC2118
  2. make IR color-color plots that can be used to find young stars and hopefully determine the age of stars. ...t the Spitzer Space Center. Luisa’s main area of interest is properties of young stars. She is particularly interested in finding out about how a star’s r
  4 KB (631 words) - 18:34, 18 July 2007
• How Do We Observe Star Formation
  ...of environment, which can significantly affect the emergent light from the young stars or protostars. ...ng the color-color plots to primary distinguish between different types of young or proto stars.
  4 KB (676 words) - 19:26, 7 February 2013
• C-WAYS Useful Links
  [[Studying Young Stars]] - wiki page on this. lots of interwoven links to other good stuff o ...nt presentation giving at GISS 2011 summarizing the NITARP 2010 paper "New Young Star Candidates in CG4 and Sa101", Rebull et all, 2011 [[File:GISS_2011_Le
  3 KB (481 words) - 23:26, 26 January 2012

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