NGC 6384

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NGC 6384
NGC 6384 HST.jpg
Hubble Space Telescope image of NGC 6384
Observation data (J2000 epoch)
Constellation Ophiuchus
Right ascension 17h 32m 24.302s [1]
Declination +07° 03 36.97 [1]
Helio radial velocity 1,665  km/s [2]
Distance 76.6 Mly (23.5 Mpc) [2]
Characteristics
Type SAB(r)bc [3]
Mass 1.05 × 1011 [3]   M
Size138,000 light years
Other designations
UGC 10891

NGC 6384 is an intermediate barred spiral galaxy located about 77 million light-years away in the northern part of the constellation Ophiuchus. It has a morphological classification of SAB(r)bc, [3] indicating that it is a weakly barred galaxy (SAB) with an inner ring structure (r) orbiting the bar, and moderate to loosely wound spiral arms (bc). [4] The galaxy is inclined by an angle of 47° to the line of sight, along a position angle of 40°. [5] The estimated mass of the stars in this galaxy is 105 billion times the mass of the Sun. [3]

Contents

At one time NGC 6384 was considered a normal galaxy with no activity in the nucleus. However, it is now classified as a transition object (T2), which is thought to be a LINER-type galaxy whose emission-line spectra is contaminated by H II regions in the nucleus. [6]

Tow supernovae have been observed in NGC 6384. On 24 June 1971, a type Ia supernova event was discovered in this galaxy at 27″ east and 20″ north of the nucleus. It reached a peak visual magnitude of 12.85 around the end of June. [7] Designated SN 1971L, it was situated along a spiral arm, suggesting that the progenitor was not a member of the older, more evolved stellar population of the galaxy. [5] On 3 May 2017, SN 2017drh (type Ia, mag. 17.9) was discovered. [8]

Related Research Articles

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<span class="mw-page-title-main">Messier 84</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 3486</span> Galaxy in the constellation Leo Minor

NGC 3486 is an intermediate barred spiral galaxy located about 27.4 million light years away in the constellation of Leo Minor. It has a morphological classification of SAB(r)c, which indicates it is a weakly barred spiral with an inner ring and loosely wound arms. This is a borderline, low-luminosity Seyfert galaxy with an active nucleus. However, no radio or X-ray emission has been detected from the core, and it may only have a small supermassive black hole with less than a million times the mass of the Sun.

<span class="mw-page-title-main">NGC 4945</span> Galaxy in the constellation Centaurus

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−0.7
×1011 M
.

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<span class="mw-page-title-main">NGC 1808</span> Galaxy in the constellation Columba

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<span class="mw-page-title-main">NGC 5962</span> Galaxy in the constellation Serpens

NGC 5962 is a spiral galaxy in the equatorial constellation of Serpens Caput. It was discovered by the Anglo-German astronomer William Herschel on March 21, 1784. The NGC 5962 galaxy is located at a distance of 120 million light years and is receding with a heliocentric radial velocity of 1,957 km/s. It is the brightest member of the eponymously-named NGC 5962 group, which overlaps with the nearby NGC 5970 group; the two groups may be gravitationally bound.

<span class="mw-page-title-main">NGC 2770</span> Spiral galaxy in the constellation Lynx

NGC 2770 is a spiral galaxy in the northern constellation of Lynx, near the northern constellation border with Cancer. It was discovered by German-born astronomer William Herschel on December 7, 1785. J. L. E. Dreyer described it as, "faint, large, much extended 150°, mottled but not resolved, 2 stars to north". NGC 2770 was the target for the first binocular image produced by the Large Binocular Telescope.

<span class="mw-page-title-main">NGC 5584</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 1084</span> Galaxy in the constellation Eridanus

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<span class="mw-page-title-main">NGC 1003</span> Galaxy in the constellation Perseus

NGC 1003 is a spiral galaxy at the western edge of the Perseus constellation. It is located at a distance of about 36 million light years from the Milky Way and is receding with a heliocentric radial velocity of 624 km/s. This galaxy was discovered by the Anglo-German astronomer William Herschel on October 6, 1784, who described it as "pretty faint, large, extended 90°±, much brighter middle, mottled but not resolved". It is a member of the NGC 1023 group of galaxies.

<span class="mw-page-title-main">NGC 2782</span> Galaxy in the constellation Lynx

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<span class="mw-page-title-main">NGC 4424</span> Spiral galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 3294</span> Galaxy in the constellation Leo Minor

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References

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  8. Transient Name Server entry for SN 2017drh. Retrieved 25 March 2023.