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Re: [APML] A new Nebula discovered in M78!!!



Even better, the new nebula is reported now to be getting brighter!!, the 'new' or variable star that's illuminating it is definitely erupting! It
might even be visible soon , who knows.
 
Keith...
 
----- Original Message -----
Sent: Tuesday, February 10, 2004 6:57 PM
Subject: [APML] A new Nebula discovered in M78!!!

Dear friends, I want to suggest you to check all your recent images of M78, since a new *bright* nebula has been just discovered near there with a 3" refractor! Here is an abstract of Central Bureau for Astronomical Telegrams #8284
 
                                                  Circular No. 8284
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
CBAT@CFA.HARVARD.EDU (science)
URL http://cfa-www.harvard.edu/iau/cbat.html  ISSN 0081-0304
Phone 617-495-7440/7244/7444 (for emergency use only)


IRAS 05436-0007
     A report was received from J. W. McNeil, Paducah, KY, of the
appearance of a new nebula in a dense region of the Lynds 1630
cloud in Orion, and apparently associated with IRAS 05436-0007, on
his unfiltered CCD images taken with a 7.6-cm refractor on Jan. 23
UT.  The object, which is located at R.A. = 5h46m14s, Decl. =
-0o05'.8 (equinox 2000.0), was then of total mag about 15-16 (with
his CCD camera's sensitivity peaking at 575 nm), but it is not
present on seven Digitized Sky Survey images from 1951 to 1991.  B.
Reipurth, University of Hawaii (UH), confirms that a faint optical
counterpart to IRAS 05436-0007 has gone into outburst and has
produced a large reflection nebulosity, based on preliminary
examination of red broadband CCD images obtained with K. Meech at
the UH 2.2-m telescope on Jan. 31.  Reipurth adds that this is a
very rare event, apparently similar to that involving IRAS
05380-0728 (cf. Reipurth and Bally 1986, Nature 320, 336).  The
outburst may be an EX-Lup-type or FU-Ori-type eruption, driven by a
sudden increase of accretion through a circumstellar disk, and thus
in urgent need of observation (see Herbig 1977, Ap.J. 217, 693;
Lehmann et al. 1995, A.Ap. 300, L9; Hartmann and Kenyon 1996, ARAA
34, 207).  Reipurth also notes that HH 22 is in the line-of-sight
of this new nebula but is not physically involved with the nebula
(Eisloeffel and Mundt 1997, A.J. 114, 280).


Some images of the discover are visible on McNeil's site:
There are traces of this nebula on images back to 2001, I checked on one of my shot taken in 1999 and there is no hint of it.
Unbelievable but sometime something in the universe changes :-)
 
Marco


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