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• 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

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