FITS and PV diagrams of the Orion A Giant Molecular Cloud
If you use these FITS data, PV diagrams and/or catalogs, please cite the corresponding
reference(s).
Orion
N2H+ integrated intensity map of the Orion A Giant Molecular Cloud
N2H+ velocity channel map (data cube) of the Orion A Giant Molecular Cloud
[0.3 km/s velocity bin, the LSR velocity is defined with respect to
the main N2H+ J = 1-0
component (F_1, F) = (2, 3)-(1, 2), contains seven hyperfine components]
N2H+ data of the Orion A Giant Molecular Cloud in random groups FITS format
[0.12 km/s velocity resolution, the LSR velocity is defined with respect to
the main N2H+ J = 1-0
component (F_1, F) = (2, 3)-(1, 2)]
HC3N integrated intensity map of the Orion A Giant Molecular Cloud
Please refer to
Tatematsu, K., Kandori, R., Umemoto, T., and Sekimoto, Y. 2008, PASJ, 60, 407
PV diagrams of N2H+ cores in the Orion A Giant Molecular Cloud
Please refer to
Tatematsu, K., Kandori, R., Umemoto, T., and Sekimoto, Y. 2008, PASJ, 60, 407
and
Tatematsu, K., Ohashi, S., Sanhueza, P., Nguyen Luong, Q., Umemoto, T., and Mizuno, N. 2016, PASJ, 68, 24
PV diagrams are drawn for the isolated hyperfine component N$_2$H$^+$ $J = 1\rightarrow0$,
$F_1$, $F$ = 0, 1$\rightarrow$1, 2, but
the velocity axis is the LSR velocity (km s$^{-1}$) corresponding to
the main N$_2$H$^+$ $J = 1\rightarrow0$
component ($F_1$, $F$ = 2, 3$\rightarrow$1, 2).
To obtain the LSR velocity corresponding to $F_1$, $F$ = 0, 1$\rightarrow$1, 2,
you need to add 8.0082 km/s.
FileName=pvX-Y.ps, with X as TUKH core number and Y=1,2,3,4 for PA=0,45,90,135 deg, respectively.
Strips for Y=2,4 are 1.414 times longer than those of Y=1,3.
CS (1-0) data cube (small)
CS (1-0) peak intensity map (0.3 km/s smoothed data)
CS (1-0) integrated intensity map
1.66 square deg map at 40 arcsec spacings with 36 arcsec beam
CS (1-0) core catalog
(tab-deliminated text format)
Please refer to
Tatematsu, K., et al. 1993, ApJ, 404, 643
CS (2-1) data cube of the Orion A Giant Molecular Cloud
CS (2-1) peak intensity map
2.63 square deg map
Please refer to
Tatematsu, K., Umemoto, T., Heyer, M.H., Hirano, N., Kameya, O.,
and Jaffe, D.T. 1998, ApJS, 118, 517
13CO (1-0) data cube (full) of the Orion A Giant Molecular Cloud
13CO (1-0) data cube (small)
13CO (1-0) peak intensity map (0.3 km/s smoothed data)
13CO (1-0) integrated intensity map
1.66 square deg map at 40 arcsec spacings with 15 arcsec beam
Tatematsu, K., et al. 1993, ApJ 404, 643 and additional data
another 13CO (1-0) data cube of the Orion A Giant Molecular Cloud
another 13CO (1-0) peak intensity map (0.3 km/s smoothed data)
another 13CO (1-0) integrated intensity map
Another smaller map at 17, 17*sqrt(2), or 34 arcsec spacings with
Nobeyama 45 m radio telescope (15 arcsec beam)
Please refer to
Hirano, N., Umemoto, T., Kameya, O., and Tatematsu, K. 1999,
unpublished data
C18O (1-0) data cube of the Orion A Giant Molecular Cloud
C18O (1-0) peak intensity map (0.3 km/s smoothed data)
C18O (1-0) integrated intensity map
Mapped at 17, 17*sqrt(2), or 34 arcsec spacings
with
Nobeyama 45 m radio telescope (15 arcsec beam)
Please refer to
Hirano, N., Umemoto, T., Kameya, O., and Tatematsu, K. 1999,
unpublished data
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