Date and Time of the Query: 2022-01-19 T03:49:06 PST
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Notes for object NGC 6015

7 note(s) found in NED.

1. 2008MNRAS.388..500E
Re:UGC 10075
UGC 10075 (NGC 6015). There is a good agreement between our H{alpha} map and
that of James et al. (2004). We detect, however, some faint emission in an outer
spiral arm to the south-east that they do not detect. Our H{alpha} rotation
curve is in good agreement with the slit spectroscopy observations of Carozzi
(1976) when correcting for the different inclinations adopted. However, her
detection was not as good, and our rotation curve is almost twice more extended,
clearly showing a slowly rising plateau beyond 50 arcsec radius. No H I velocity
map is available in the literature but the width of the H I profile at 20 per
cent (315 km s^-1^ from Springob et al. 2005, 310 km s^-1^ from Bottinelli et
al. 1990) is in good agreement with our H{alpha} velocity field amplitude. It
has been observed in CO by Braine et al. (1993) who find a strong CO emission at
40 arcsec (2.7 kpc) from the centre.

2. 2007AJ....134.2286H
Re:KIG 0710
CIG 710: The galaxy was classified as SA(s)cd (NED). The optical and composed
JHK images show an elongated central region resembling a bar. The photometric I-
and JHK-band ({epsilon} and P.A.) profiles also show weak evidence of a bar. The
total (B - V) color is representative of SdSm types. We classify this galaxy as

3. 1994CAG1..B...0000S
Re:NGC 6015
June 6/7, 1970
103aO + GG385
20 min
The multiple-arm pattern of NGC 6015
starts at the center in a prototype (s)-type
configuration. There is no evidence of a central
bulge. The nucleus is small, characteristic of the
Sc morphology. The redshift of NGC 6015 is
v_o = 1018 km/s.

4. 1993A&AS...97..887B
Re:NGC 6015
NGC 6015 is a new detection but was observed by Rickard (cf. Verter 1985)
in CO(1-0). The important feature is the strong CO emission at 40" (2.7
kpc) from the center. CO was detected in the center but given the
inclination (65^deg^) some of it could be from the off-center emission.
The CO(2-1)/CO(1-0) ratio is unclear in the center as the CO(2-1)
intensity decreases when the CO(1-0) line width is used as the window
rather than the CO(2-1) line width. At 40" from the center the ratio is
0.9 for the unconvolved beams. We have not found a "ring" classification
for this galaxy. We believe that there is molecular gas, in the nucleus
with a deficiency from radii of about 0.7 kpc to 2kpc.

5. 1976RC2...C...0000d
Re:NGC 6015
Rotation Curve and Systemic Velocity:
Astr. Ap., 8, 364, 1970.
HII Regions:
Ap. J., 194, 559, 1974.
Ap. J. Suppl., 27, No. 239, 1974.
Distance Modulus:
Ap. J., 194, 559, 1974.

6. 1973UGC...C...0000N
Re:UGC 10075
SA(s)cd (de Vaucouleurs), Sc+ (Holmberg)

7. 1964RC1...C...0000d
Re:NGC 6015
Very small, bright nucleus in a complex center with many dark lanes. Many
knotty arms in a bright lens. Pseudo (R): 5.2 arcmin x 1.8 arcmin.
Heidelberg Veroff. Vol. 9, 1926 dimensions are for the bright part only.

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