\cgidef{-tex -cat -bib -oglu}
\title{Notes from B. Skiff about MacConnell's stars}
\begin{BODY bgcolor="#ededff"}
\JavaPop

\centerline{{\large\bf Notes concerning 
     {\fg{red4}IRAS Point Source Identifications} (Cat. III/170)}\br
     {\em by B. Skiff}}

%%% Note: file may be used from VizieR -- in this case PATH_INFO=Vgrep
\def\Aviz#1{\ifmatch{*Vgrep*}{\env{PATH_INFO}}{#1:\quad}\else%
\A{/viz-bin/VizieR?-source=III/170B\&IRAS===#1}{{\fg{red4}#1}}\fi}

\begin{itemize}

\item
\Aviz{05385+3231} 
   IRAS coords lie between this star and \object{DO 11468}(K5);
   MSX6C shows similar A-band flux for both stars.

\item
\Aviz{06303+0127}
    eastern of two red stars contributing equally to the IRAS source;
    western star = \object{DO 1628}:  6 32 51.80 +01 25 37.5 (U), DO type M1.

\item
\Aviz{06341-0335}
    earlier than type M2/3 but reddened, per MacC email 2005Nov7. 

\item       
\Aviz{06520+0018}
    this is a reflection nebula classified in error as type M10?.

\item       
\Aviz{07033-1215}
    MacC notes indicate two stars of type M8, but only one red star is
    evident on visible-light and 2MASS images.

\item       
\Aviz{07152-1841}
    nearby \object{HD 56747} probably contributes to IRAS flux.

\item       
\Aviz{07339-3000}
    not a red star:  type M5? probably an error per MacC email of 2005Jun27. 
    The IRAS source is probably not nearby \object{CGCS 1793}, 
    though a poor IRAS position is not excluded.

\item       
\Aviz{07363-0838}
    second red star at 7 38 47.5 -08 45 29 (J2000) contributes to IRAS flux,
    however no TiO present per MacC e-mail 2005Jun27.

\item       
\Aviz{07431-2919}
    original type (M6:) revised per MacC re-examination of plates 2005Jul1,
    and definitely not a carbon star.

\item       
\Aviz{07434-2927}
    carbon, not type M5:, per MacC re-examination of plates 2005Jul1.

\item       
\Aviz{07588-2418}
    MacC re-examination of plates 2005Jul13 suggests strong CN, but not 
    obviously a carbon star.

\item       
\Aviz{08368-4137}
    another fainter red star at 8 38 40.84 -41 48 51.1 (U) contributes to the 
    IRAS flux.

\item       
\Aviz{09237-5429}
    type for M7 star per MacC e-mail 2006Mar1.

\item       
\Aviz{09350-5314}
    MacC re-examination of plates 2006Apr3:  the forbidden emission lines 
    probably mistaken for TiO bandheads; IR CaII triplet seems to be in emission
    also.

\end{itemize}
\CDStail{\thefile}