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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
• IC 417 Bigger Picture and Goals
  We have WISE data for a patch of sky likely to harbor young stars around IC 417. ...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
  9 KB (1,543 words) - 22:24, 17 April 2015
• Matt Piper
  Our group is looking into the formation of Young Stellar Objects (YSOs) near Bright Rimmed Clouds (BRCs). We want to learn
  1 KB (225 words) - 21:08, 19 June 2012
• Color selection
  Most of what we have right now focuses on young stars, but these kinds of techniques can be (and are) used for any class of
  2 KB (266 words) - 20:21, 11 August 2020
• StarsAtYerkes AAS 2012
  ...Institute)]] describes their discovery of a total of 19 previously unknown Young Stellar Objects (YSOs) in BRC 27 and 8 YSOs in BRC 34. The groups Educatio
  4 KB (584 words) - 22:11, 23 January 2012
• SED plots introduction
  ...| page on studying young stars]] has examples of SEDs for, you guessed it, young stars. ...m the (still uncompleted) star formation process. On that page ([[Studying Young Stars]]), it has several schematic SEDs included partway down the page. [ht
  8 KB (1,406 words) - 17:05, 31 July 2020
• Gutermuth color selection
  ...ious contaminants to create a short list of sources that might actually be young stars. ...gnitude spaces all at once (by computer) to get a first guess at a list of young stars. Koenig et al. (2011) extended this method to the WISE bands. Here w
  7 KB (1,203 words) - 20:14, 20 April 2015
• IC 2118 Current Research Activities
  ====[[General Background on young stars]]====
  669 bytes (85 words) - 18:49, 6 March 2008
• Wendi's table of all data sources
  ...luster members]], originally known as "Luisa’s Table of Characteristics of Young Stars for Determining Cluster Members", may be of some interest.'' ...uce number of foreground/background objects by requiring X-ray detections. Young stars are bright in X-rays because they are rotating quickly and therefore
  4 KB (701 words) - 23:24, 29 May 2013
• LLAMMa Bigger Picture and Goals
  ''Most succinct:''  We will be looking for new candidate young stars in Ceph C using X-rays, optical, and IR data.  ...C. It has not been well-studied to date. Our goal is to find new candidate young stars in this region. We have data from:
  10 KB (1,779 words) - 20:19, 18 February 2016
• Color-Magnitude and Color-Color plots Overview
  =Color-Color plots and Young Stars= ...tool in (a) finding the young stars, and (b) making a guess at the age of young stars. Using Spitzer colors, we can do this more easily than in many other
  9 KB (1,583 words) - 18:15, 23 June 2021
• C-CWEL Bigger Picture and Goals
  We have WISE data for a patches of sky likely to harbor young stars around 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
  11 KB (1,936 words) - 16:11, 28 February 2013
• Manipulating Numerical Data and Applying Rules to Create Lists and Plots with Excel
  ...on this CG4 project are blind to the infrared light we used to detect the young stellar objects embedded in nebular clouds of dust and gas. As is common i ...ds for analysis, and to form user-generated filters to separate potential "young stellar objects" from other light sources. Therefore, users are able to pe
  4 KB (649 words) - 22:53, 8 January 2011
• Resolution and YSOs
  ...ot of time in the study of YSOs talking about the rings of dust around the young stars, and how they can become more prominent at longer wavelengths. When y ...the sources seen in MIPS. '''''THESE ARE NOT THE DUST RINGS AROUND THESE YOUNG STARS'''''. I cannot emphasize this enough. There are only about 10 source
  6 KB (1,069 words) - 01:42, 28 July 2020
• Finding cluster members
  This document is also known as "Luisa’s Table of Characteristics of Young Stars for Determining Cluster Members". ...tire lifetime, and so it is with stars. You have to seek out the group of young stars/humans in order to study their development.
  19 KB (3,216 words) - 23:02, 25 January 2024
• Luisa's BRC task notes
  *stars vary, especially young stars. this guy probably flared in Ha (e.g., ate something out of its disk) ...able is a GOOD thing, because variability is one of the characteristics of young stars.
  4 KB (662 words) - 17:00, 24 June 2011
• 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
• C-CWEL Useful Links
  [[Studying Young Stars]] - wiki page on this. lots of interwoven links to other good stuff o
  2 KB (296 words) - 22:20, 12 January 2013
• Coherent ideas of what to do with these pieces
  ...color selections? Would your method work if your catalog had a mixture of young stars and field stars?
  7 KB (1,074 words) - 16:32, 6 October 2022
• Spitzer Space Telescope
  *'''YOUNG STELLAR OBJECTS, PROTOPLANETARY & DEBRIS DISKS''' Spitzer has been useful in identifying the location of young stellar objects (YSO's). Because YSO's initially develop behind a thick vei
  6 KB (928 words) - 21:23, 29 July 2020
• LLAMMa Useful Links
  [[Studying Young Stars]] - wiki page on this. lots of interwoven links to other good stuff o
  2 KB (324 words) - 17:05, 19 January 2016
• Another CMD explanation attempt
  ...ain sequence. You can use catalogs like this to establish where you expect young stars (or
  5 KB (861 words) - 19:46, 11 August 2020
• CephC-LABS Useful Links
  [[Studying Young Stars]] - wiki page on this. lots of interwoven links to other good stuff o
  2 KB (345 words) - 22:14, 10 January 2017
• SHIPsProposal
  ** What is the evidence for young stars in NGC 281? (MELISSA) |IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281
  6 KB (884 words) - 11:19, 8 March 2013
• Specific IC 2118 information
  ...e-main sequence stellar evolution in this cluster. We want to (a) find the young stars, and (b) compare star formation in this cluster with others from diff
  4 KB (636 words) - 18:57, 23 February 2007
• ProtostarsInNGC281
  ...HII emission region Sharpless 184 of diameter 20 arcminutes containing the young galactic cluster IC 1590 centered about the OB star trapezium system HD5005 • HII emission containing the young galactic cluster IC 1590, OB star trapezium system HD5005 with what appears
  4 KB (650 words) - 22:53, 9 December 2013
• CG4 Spring work
  *[[Studying Young Stars]] -- including page on SEDs that is linked from there.
  3 KB (431 words) - 23:30, 21 April 2010
• Future Research Project Ideas
  *[http://www.butrousfoundation.com/ysjournal/] "Young Scientists is a free online journal for scientists aged 12-20. The journal
  3 KB (427 words) - 15:08, 20 May 2013
• WISE
  ...he sky for 'cool' objects. These include brown dwarfs, debris discs around young stars, asteroids, comets, and ULIRGs (Ultra Luminous Infrared Galaxies).
  2 KB (382 words) - 02:37, 22 January 2013
• 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
• IC 417 Useful Links
  [[Studying Young Stars]] - wiki page on this. lots of interwoven links to other good stuff o
  3 KB (452 words) - 19:47, 10 January 2015

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