RE: OR: Fremont Peak 1/29/03

From: Bob Czerwinski (bczerwin@No-Spam)
Date: Fri Jan 31 2003 - 00:14:52 MST

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    Thanks for all the info and for answering my questions, Steve! You just
    saved me a great deal of weekend homework. <grin>

    Looking forward to reading your _Sky_&_Telescope_ article when it's
    published, too!

    ...Bob...

    > -----Original Message-----
    > From: sf-bay-tac-bounces@No-Spam
    > [mailto:sf-bay-tac-bounces@No-Spam] On Behalf Of Steve Gottlieb
    > Sent: Thursday, January 30, 2003 5:20 PM
    > To: The Astronomy Connection
    > Subject: Re: [TAC] OR: Fremont Peak 1/29/03
    >
    >
    > In a message dated 1/30/03, Bob Czerwinski writes:
    >
    > > I ran into problems locating several items, a couple in Leo
    > and one in
    > > CVn. Although I'm quite certain I was in the correct positions, I
    > > couldn't locate NGC 3498 and 3616 in Leo, nor could I
    > properly identify
    > > 4401 in Virgo. Here were the problems:
    > >
    > > 3498: Assuming the coordinates I have are fine, I was able to locate
    > > both 3489 and 3485 nearby. 3498 should have formed a nice
    > triangle with
    > > these two. A surface brightness problem?
    >
    > Well, the problem here is that NGC 3498 probably does not
    > exist!! It was
    > reported by William Herschel (III 75) and described as "eF,
    > not S. I had
    > some doubt and put on 240x, but there being no stars very
    > near to it, I could
    > not adjust the focus, and therefore could not verify it."
    >
    > And later highly-respected 19th century observers, including Heinrich
    > d'Arrest and Guillaume Bigourdan, could not find it again.
    > In the 1926, Karl
    > Reinmuth reported (based on a photographic survey of the
    > Herschel objects)
    > that "In Dreyer's place is vF triple star, *14.7, *14.7, *16,
    > a *14.7 f 1.8'
    > of *16." That's likely what confused Herschel - a faint
    > triple star! Here's
    > the position: 11 01 41.5 +14 21 04
    >
    >
    > > 3616: Should have been just outside of the field with Theta
    > Leonis, and
    > > in the same field with NGC 3596. Again, if the coordinates
    > are correct,
    > > maybe another SB problem?
    >
    > This is another lost William Herschel discovery (III 76)
    > which could not be
    > recovered by Bigourdan with the 12-inch refractor of the
    > Paris Observatory or
    > in later photographic searches (Max Wolf and Reinmuth). This
    > may have have
    > just a single faint star at 11 18 08.9 +14 45 53, but I'm
    > surprised it is
    > listed is some source as a galaxy.
    >
    >
    > > 4401: This is entirely different from the others.
    > Coordinates put it
    > > right in the middle of the area occupied by NGC 4395, a
    > huge haze with
    > > two or three HII regions. I identified 4395 with no
    > problem, which was
    > > best viewed with relatively low magnification. Is 4401
    > just one of the
    > > HII regions, much like NGC 604 in M33? Is there a separate
    > galaxy in
    > > that mess?
    >
    > Ah, this is a very interesting, active galaxy who a number of
    > HII knots which
    > received separate NGC designation. It is a bit difficult to
    > sort out of the
    > individual HII masses (which may look like individual
    > galaxies!), but there
    > is only one galaxy here. This one requires very good
    > transparency and seeing
    > to make some sense of the view (at least in my 17.5"):
    >
    > 17.5" (5/15/99): N4395 is a chaotic galaxy dominated by
    > several bright HII
    > regions. At 100x, the large low surface brightness glow is
    > clearly clumpy
    > with a couple of faint knots evident on the east side of the
    > haze. At 220x,
    > the glow of the galaxy is more difficult to view and several
    > nonstellar knots
    > and a couple of very faint superimposed stars are more prominent. The
    > brightest HII region is N4401, located 2' SE of the core,
    > ~25" in size, with
    > a second smaller 15" knot (N4400) close south. The core of
    > the galaxy appears
    > as an ill-defined low surface brightness glow, larger than
    > the individual HII
    > knots. A mag 14.5 star is superimposed NE of the core. On
    > the SW side of the
    > core is a third difficult knot, about 15" in diameter (N4399)
    > requiring
    > averted vision to confirm.
    >
    > By the way, I recently submitted an article to Sky & Tel on
    > the problems of
    > NGC identifications and the craft of catalogue sleuthing -
    > should be coming
    > up later this year.
    >
    > Steve Gottlieb
    >
    >
    >



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