Dictionary of Nomenclature of Celestial Objects
(Last update: 06-Dec-2017)

Result of query: info cati HH$

Details on Acronym:   HH
   HH (Herbig-Haro obj.) ***** Avoid the usage of HH, prefer [ASS79] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   HH
   HH (Harris+Geisler) ***** Avoid the usage of HH, prefer [BBP2008] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   HH
   HH (Herbig Haro obj.) Write:<<HH NNNNA>>
<<HH NNNNA'>>
<<HH NNNNa>>
<<HH NNNNANN>>
<<HH NNNNAA>>
<<HH NNNNAW>>
<<HH NNNNAaNN>>
<<HH NNNNaN>>
<<HH NNNNWA>>
<<HH NNNNWW>>
<<HH NNNNWWW>>
<<HH NNNNWWN>>
<<HH NNNNWWNA>> N: 1120 Object:HH  (SIMBAD class: HH = Herbig-Haro Object) Note:Numerous subdivisions (may be A, AN, AW where W stands for West or South or.., AA, WA, WW, WWW, etc...).
Begins to be published in 1974.
Ref. 1988A&AS...74..431V is a compilation.
Catalogue is on electronic form, catalogue V/104/: (Nos 1-478) with missing numbers, some of these missing numbers being found in the literature.
Nos up to 1107 are also found in the literature.
See also [SBW2010] for the candidate jets of Smith, Bally & Walborn (2010MNRAS.405.1153S, table 3). =E=Catalogue in electronic form as V/104
Details on Acronym:   HH
   HH (Smith+Bally+Walborn, 2010) ***** Avoid the usage of HH, prefer [SBW2010] Originof the Acronym: S = Created by Simbad, the CDS Database
Details on Acronym:   OHH
   OHH (Ohio univ., H stands for 7th hour of RA, H stands for High-Vel.) ***** Avoid the usage of OHH, prefer Ohio Originof the Acronym: L = Found in the literature
Details on Acronym:   Cl* NGC 104 HH
   Cl* NGC 104 HH (Hesser+Hartwick) Write:<<Cl* NGC 104 HH NNNN # 4 digits>> N: about 1500 Object:*inCl Ref:=1977ApJS...33..361H byHESSER J.E. , HARTWICK F.D.A. Astrophys. J., Suppl. Ser., 33, 361-389 (1977) Metal-rich globular clusters in the galaxy. V. A photometric study of 47 Tucanae. oTables 1-4: <Cl* NGC 104 HH NNNN> N=about 1500.
Details on Acronym:   Cl* NGC 1817 HH
   Cl* NGC 1817 HH (Harris+Harris) Write:<<Cl* NGC 1817 HH NNNN # 4 digits>> N: 86+126+147 Object:*inCl Rem:In the format 'NNNN' (always a 4 digits format), the first
digit stands for rings Nos 1 to 3. Ref:=1977AJ.....82..612H byHARRIS G.L.H. , HARRIS W.E. Astron. J., 82, 612-619 (1977) The Hyades-age cluster NGC 1817. oFig.1, Table III: <Cl* NGC 1817 HH NNNN> (Nos 1001-1086, 2001-2126, 3001-3147).
Details on Acronym:   Cl* NGC 2660 Hart
   Cl* NGC 2660 Hart (Hartwick+) ====>Equivalent to: Cl* NGC 2660 HH
Details on Acronym:   Cl* NGC 2660 HH
   Cl* NGC 2660 HH (Hartwick+Hesser) Write:<<Cl* NGC 2660 HH 90NN # 4 digits>>
<<Cl* NGC 2660 HH NNNN # 4 digits>>
<<Cl* NGC 2660 HH A>> N: 39+349+13 Object:*inCl Rem:Table 1: sequence *, format 90NN

Table 2: format NNNN, always 4 digits,
first digit: quadrant (I to IV),
second digit: ring 1 or 2,
two last digits NN: running number in each sector. Ref:=1973ApJ...183..883H byHARTWICK F.D.A. , HESSER J.E. Astrophys. J., 183, 883-897 (1973) NGC 2660 and its nearby carbon star. oTable 1: <Cl* NGC 2660 HH 90NN> (Nos 9001-9039). Table 2: <Cl* NGC 2660 HH NNNN> N=349 among (Nos 1101-4271). Tables 4, 5: <Cl* NGC 2660 HH A> N=13 among (Nos A-Z).
Details on Acronym:   Cl* NGC 4372 HH
   Cl* NGC 4372 HH (Hartwick+Hesser) Write:<<Cl* NGC 4372 HH NN>>
<<Cl* NGC 4372 HH NNNN>> N: 30+338 Object:*inCl Ref:=1973ApJ...186.1171H byHARTWICK F.D.A. , HESSER J.E. Astrophys. J., 186, 1171-1178 (1973) The color-magnitude diagram of the metal-poor southern globular cluster NGC 4372. oTable 2: <Cl* NGC 4372 HH NN> (Nos 1-30). Table 3: <Cl* NGC 4372 HH NNNN> N=338 among (Nos 1009-4225).
Details on Acronym:   Cl* NGC 6193 HH
   Cl* NGC 6193 HH (Herbst+Havlen) ====>Equivalent to: [HH77]
Details on Acronym:   Cl* NGC 6304 HH
   Cl* NGC 6304 HH (Hesser+Hartwick) ====>Equivalent to: NGC 6304
Details on Acronym:   Cl* NGC 6352 HH
   Cl* NGC 6352 HH (Hartwick+Hesser) Rem:Table 3 ====>Equivalent to: NGC 6352
Details on Acronym:   Cl* NGC 6352 HH
   Cl* NGC 6352 HH (Hartwick+Hesser) Write:<<Cl* NGC 6352 HH A>>
<<Cl* NGC 6352 HH NN>> Object:*inCl Rem:Tables 1 and 2. Ref:=1972ApJ...175...77H byHARTWICK F.D.A. , HESSER J.E. Astrophys. J., 175, 77-88 (1972) The abnormally metal-rich globular cluster NGC 6352. oTable 1: <Cl* NGC 6352 HH A> (Nos A-J). Table 2, Fig.1: <Cl* NGC 6352 HH NN> (Nos 1-64). Table 3: <NGC 6352 NNN> (Nos 1-74, 101-510).
Details on Acronym:   Cl* NGC 6388 HH
   Cl* NGC 6388 HH (Hazen+Hesser) Write:<<Cl* NGC 6388 HH FN>> N: 4 Object:V* Rem:N=4 stars (Nos F1-F4), outside the tidal radius of the cluster. Ref:=1986AJ.....92.1094H byHAZEN M.L. , HESSER B.H. Astron. J., 92, 1094-1099 (1986) The variable stars in the globular cluster NGC 6388. oTable II: <Cl* NGC 6388 Saw VNN> (Nos V13-V26) added. Table II: <Cl* NGC 6388 HH FN> (Nos F1-F4).
Details on Acronym:   Cl* NGC 6388 HH
   Cl* NGC 6388 HH (Hazen+Hesser) ====>Equivalent to: Cl* NGC 6388 Saw
Details on Acronym:   Cl* NGC 6441 HH
   Cl* NGC 6441 HH (Hesser+Hartwick) ====>Equivalent to: NGC 6441
Details on Acronym:   Cl* NGC 6441 HH
   Cl* NGC 6441 HH (Hesser+Hartwick) Write:<<Cl* NGC 6441 HH A>> N: 7 Object:*inCl Ref:=1976ApJ...203...97H byHESSER J.E. , HARTWICK F.D.A. Astrophys. J., 203, 97-112 (1976) Metal-rich globular clusters in the galaxy. III. The "X-ray" globular clusters NGC 6441. oTable I: <Cl* NGC 6441 HH A> (Nos B-I). Table I: <NGC 6441 NNN> N=37 among (Nos 1-115). Table II: <NGC 6441 NNNN> N about 700 among (Nos 1201-4505).
Details on Acronym:   Cl* NGC 663 HH
   Cl* NGC 663 HH (Hopmann+Haidrich) Write:<<Cl* NGC 663 HH a>>
<<Cl* NGC 663 HH NNN>> N: 17+168 Object:*inCl Ref:=1959MiWie..10..129H byHOPMANN J. , HAIDRICH K. Mitt. Univ. Sternw. Wien, 10, 129-154 (1959) Der galaktische Sternhaufen NGC 663. oTable 1: <Cl* NGC 663 HH a> (Nos a-g). Catalog: <Cl* NGC 663 HH NNN> (Nos 1-168).
Details on Acronym:   Cl* NGC 663 Wi
   Cl* NGC 663 Wi (Wien obs.) ====>Equivalent to: Cl* NGC 663 HH
Details on Acronym:   Cl* NGC 7129 HH
   Cl* NGC 7129 HH (Herbig-Haro) Write:<<Cl* NGC 7129 HH N>> N: 4 Object:*inCl Rem:Table 1, HH1 to 4. Stars 1, 2, 3 are 'Cl* NGC 7129 MEG N' Ref:=1993A&A...271..564M byMIRANDA L.F. , EIROA C., GOMEZ DE CASTRO A.I. Astron. Astrophys., 271, 564-573 (1993) New Herbig-Haro objects and pre-main sequence stars in the star formation region NGC 7129. oTable 1: <Cl* NGC 7129 MEG N> (Nos 1-3), <Cl* NGC 7129 HH N> (Nos 1-4) Originof the Acronym: A = Assigned by the author(s)
Details on Acronym:   Cl* Palomar 14 HH
   Cl* Palomar 14 HH (Holland+Harris) Write:<<Cl* Palomar 14 HH NNN>> N: 327 Object:*inCl Ref:=1992AJ....103..131H byHOLLAND S. , HARRIS W.E. Astron. J., 103, 131-141 (1992) A photometric study of the "second parameter" globular cluster Palomar 14. oTable 3: <Cl* Palomar 14 HH NNN> (Nos 1-327).

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