Talk:CG4 Spring work

For Apr 14: KEVIN -- Reipurth and Pettersson 1993

http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?1993A%26A...267..439R&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf

Main Point

Found 8 new YSOs in Gum Nebula (near CG4 and Sa101 and CG13) using IR photometry, UBV photometry and spectroscopy.

High Level Summary

Surveyed 5 fields with 15 cometary globules Found 8 new YSOs Confirmed one previous YSO

Equipment Used

 Ha spectroscopy                      CTIO 60/90cm Curtis Schmidt telescope with 6deg prism    1-2hrs
 JHK IR photometry (sort of like us)  ESO 1m        J-H and H-K
 UBV photometry (like us)             ESO 1m
 Point source spectroscopy            ESO 1.52m and 3.6m        3700A to 7000A                    10-40 min

found there are different ages (spectra and movement away from globule) Found late-type premain sequence stars

Identified spectral type using spectra ruled out forground/background with spectra and

Most Interesting

Introduction: Good description of cometary nebulae Good rundown of CG formation theory

1.  OB starformed nearby and the UV radiation scrunched and eroded nearby nebula (some evidence in this paper for this method)
2.  or SN went off nearby and shockwave scrunched and eroded nearby nebula

CG4 might have been evaporating for 1,000,000years

CG4 might have been a shade for Sa101 to hide behind. Until the CG4 evaporation may have started >1,000,000 years ago. In faint background stars they found stars becoming more prominent as they used longer wavelength filters (good for us)

Spectral classes M3 to K7 M2, M3-4, K7-M0, K7, K2-5, K5, M1-2, K2

Not sure about this

Quesitons and Kevin trying to dodge the questions TiO and MgH using the width and

Ha

width of line (spinning?)

Balmer series forbidden [OI] linesat 6300 and 6363A prominent absorption at 5577A absorbtion trough at 6200A deeper

I agree with this

found eight new YSOs in the area confirmed one previous YSO found there are different ages (spectra and movement away from globule) Found late-type premain sequence stars

I disagree with this

found there are different ages (spectra and movement away from globule) probably continuous (from 8 stars?)

Why we should care

found seven new YSOs in the area confirmed one previous YSO Used some of the same techniques we will Found YSOs and confirmed previous ones Found faint background stars getting more prominent in longer wavelength filters Not all CG had star formation but CG4 was one that had some nearby

For Apr 21: VIVIAN -- Kim et al 2003

http://adsabs.harvard.edu/abs/2003csss...12..799K Full Paper link click here. [1]

For Apr 28: CHELEN -- Kim 2005

http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2003ASPC..287..275K&data_type=PDF_HIGH&whole_paper=YES&type=PRINTER&filetype=.pdf

For May 5: CAROLYN -- Choudhury and Bhatt 2008

http://arxiv.org/PS_cache/arxiv/pdf/0811/0811.4389v1.pdf

   the ADS entry is http://adsabs.harvard.edu/abs/2009MNRAS.393..959C 
   and I downloaded the real journal article for you (easier to read!) here: media:choud.pdf