NGC 6242: Difference between revisions
replaced image |
Praemonitus (talk | contribs) Expand the article and add refs. |
||
Line 1: | Line 1: | ||
{{Infobox open cluster |
{{Infobox open cluster |
||
| |
| name = NGC 6242 |
||
| |
| image = NGC 6242 DECaPS DR2.jpg |
||
| image_size = 250 |
|||
| name = [[New General Catalogue|NGC]] 6242 |
|||
| caption = NGC 6242 |
|||
| type = [[Open Cluster]] |
|||
| |
| credit = DECaPS |
||
| epoch = [[J2000]] |
|||
| ra = {{RA|16|55.6}}<ref name="simbad">{{cite simbad |
|||
| constellation = [[Scorpius (constellation)|Scorpius]] |
|||
| title=NGC 6242 |
|||
| ra = {{RA|16|55|30.7}}<ref name=Tarricq_et_al_2021/> |
|||
| access-date=2007-04-24}}</ref> |
|||
| dec = {{DEC| |
| dec = {{DEC|−39|28|26}}<ref name=Tarricq_et_al_2021/> |
||
| dist_ly = {{cvt|1.335|±|0.163|kpc|kly|order=flip|lk=on}}<ref name=Spina_et_al_2021/> |
|||
| dist_ly = |
|||
| dist_pc = |
| dist_pc = |
||
| appmag_v = |
| appmag_v = 6.4<ref name=Crossen_Rhemann_2012/> |
||
| size_v = {{val|9|ul=arcminute}}<ref name=Crossen_Rhemann_2012/> |
|||
| size_v = |
|||
| radius_ly = |
| radius_ly = <!-- Radius in light years, dependent on distance --> |
||
| mass_msol = <!-- Cluster mass in solar masses: {{val|#.##|ul=solar mass}} --> |
|||
| absmag_v = |
|||
| age = 77.6<ref name=Spina_et_al_2021/> Myr |
|||
| constellation = [[Scorpius (constellation)|Scorpius]] |
|||
| notes = |
| notes = <!-- Unusual features --> |
||
| names = {{Odlist | NGC=6242 | Cr=317 }}<ref name="simbad"/> |
|||
| names = [[Collinder catalogue|Cr]] 317 |
|||
}} |
|||
|image_size=250|credit=DECaPS}} |
|||
[[File:NGC 6242 map.png|thumbnail|Map showing the location of NGC 6242]] |
[[File:NGC 6242 map.png|thumbnail|Map showing the location of NGC 6242]] |
||
'''NGC 6242''' is an [[open cluster]] in the [[constellation]] [[Scorpius (constellation)|Scorpius]]. |
|||
'''NGC 6242''' is an [[open cluster]] of stars in the southern [[constellation]] [[Scorpius (constellation)|Scorpius]]. It can be viewed with binoculars or a telescope at about 1.5° to the south-southeast of the double star [[Mu Scorpii]].<ref name=Crossen_Rhemann_2012/> This cluster was discovered by French astronomer [[Nicolas-Louis de Lacaille]] in 1752 from South Africa.<ref name=Jones_1969/> It is located at a distance of approximately {{cvt|1335|pc|ly|order=flip|lk=on}} from the Sun,<ref name=Spina_et_al_2021/> just to the north of the Sco OB 1 association.<ref name=Sana_et_al_2006/> The cluster has an estimated age of 77.6 million years.<ref name=Spina_et_al_2021/> |
|||
A [[microquasar]] with the designation [[GRO J1655-40]] is located in the vicinity of NGC 6242 and is moving away from the cluster with a runaway space velocity of {{val|112|18|u=km/s}}. It may have originated in the cluster during a supernova explosion {{val|2.2|e=5|u=year|p=~}} ago.<ref name=Combi_et_al_2007/> |
|||
==References== |
==References== |
||
{{Reflist |
{{Reflist|refs= |
||
<ref name="simbad">{{cite simbad |
|||
| title=NGC 6242 |
|||
| access-date=2007-04-24 }}</ref> |
|||
<ref name=Tarricq_et_al_2021>{{cite journal |
|||
| title=3D kinematics and age distribution of the open cluster population |
|||
| display-authors=1 | last1=Tarricq | first1=Y. |
|||
| last2=Soubiran | first2=C. | last3=Casamiquela | first3=L. |
|||
| last4=Cantat-Gaudin | first4=T. | last5=Chemin | first5=L. |
|||
| last6=Anders | first6=F. | last7=Antoja | first7=T. |
|||
| last8=Romero-Gómez | first8=M. | last9=Figueras | first9=F. |
|||
| last10=Jordi | first10=C. | last11=Bragaglia | first11=A. |
|||
| last12=Balaguer-Núñez | first12=L. | last13=Carrera | first13=R. |
|||
| last14=Castro-Ginard | first14=A. | last15=Moitinho | first15=A. |
|||
| last16=Ramos | first16=P. | last17=Bossini | first17=D. |
|||
| journal=Astronomy & Astrophysics |
|||
| volume=647 | at=id. A19 | date=March 2021 |
|||
| doi=10.1051/0004-6361/202039388 | arxiv=2012.04017 |
|||
| bibcode=2021A&A...647A..19T }}</ref> |
|||
<ref name=Crossen_Rhemann_2012>{{cite book |
|||
| title=Sky Vistas, Astronomy for Binoculars and Richest-Field Telescopes |
|||
| first1=Craig | last1=Crossen | first2=Gerald | last2=Rhemann |
|||
| page=52 | publisher=Springer Vienna |
|||
| isbn=9783709106266 | year=2012 |
|||
| url=https://www.google.com/books/edition/Sky_Vistas/3vELBwAAQBAJ?gbpv=1&pg=PA52 }}</ref> |
|||
<ref name=Jones_1969>{{cite journal |
|||
| title=The search for the nebulae - VI |
|||
| last=Jones | first=K. G. |
|||
| journal=Journal of the British Astronomical Association |
|||
| volume=79 | pages=213–222 | date=March 1969 |
|||
| bibcode=1969JBAA...79..213J }}</ref> |
|||
<ref name=Spina_et_al_2021>{{cite journal | display-authors=1 |
|||
| title=The GALAH survey: Tracing the Galactic disc with open clusters |
|||
| last1=Spina | first1=L. | last2=Ting | first2=Y. -S. |
|||
| last3=De Silva | first3=G. M. | last4=Frankel | first4=N. |
|||
| last5=Sharma | first5=S. | last6=Cantat-Gaudin | first6=T. |
|||
| last7=Joyce | first7=M. | last8=Stello | first8=D. |
|||
| last9=Karakas | first9=A. I. | last10=Asplund | first10=M. B. |
|||
| last11=Nordlander | first11=T. | last12=Casagrande | first12=L. |
|||
| last13=d'Orazi | first13=V. | last14=Casey | first14=A. R. |
|||
| last15=Cottrell | first15=P. | last16=Tepper-García | first16=T. |
|||
| last17=Baratella | first17=M. | last18=Kos | first18=J. |
|||
| last19=Čotar | first19=K. | last20=Bland-Hawthorn | first20=J. |
|||
| last21=Buder | first21=S. | last22=Freeman | first22=K. C. |
|||
| last23=Hayden | first23=M. R. | last24=Lewis | first24=G. F. |
|||
| last25=Lin | first25=J. | last26=Lind | first26=K. |
|||
| last27=Martell | first27=S. L. | last28=Schlesinger | first28=K. J. |
|||
| last29=Simpson | first29=J. D. | last30=Zucker | first30=D. B. |
|||
| journal=Monthly Notices of the Royal Astronomical Society |
|||
| year=2021 | volume=503 | issue=3 | page=3279 |
|||
| doi=10.1093/mnras/stab471 |arxiv=2011.02533 |
|||
| bibcode=2021MNRAS.503.3279S }}</ref> |
|||
<ref name=Combi_et_al_2007>{{cite journal |
|||
| title=New evidence on the origin of the microquasar GRO J1655-40 |
|||
| display-authors=1 | last1=Combi | first1=J. A. |
|||
| last2=Bronfman | first2=L. | last3=Mirabel | first3=I. F. |
|||
| journal=Astronomy and Astrophysics |
|||
| volume=467 | issue=2 | date=May 2007 | pages=597–602 |
|||
| doi=10.1051/0004-6361:20077156 | arxiv=astro-ph/0703674 |
|||
| bibcode=2007A&A...467..597C }}</ref> |
|||
<ref name=Sana_et_al_2006>{{cite journal |
|||
| title=An XMM-Newton view of the young open cluster NGC 6231. I. The catalogue |
|||
| display-authors=1 | last1=Sana | first1=H. |
|||
| last2=Gosset | first2=E. | last3=Rauw | first3=G. |
|||
| last4=Sung | first4=H. | last5=Vreux | first5=J. -M. |
|||
| journal=Astronomy and Astrophysics |
|||
| volume=454 | issue=3 | date=August 2006 | pages=1047–1063 |
|||
| doi=10.1051/0004-6361:20053224 | arxiv=astro-ph/0603783 |
|||
| bibcode=2006A&A...454.1047S }}</ref> |
|||
}} |
|||
==External links== |
==External links== |
Revision as of 16:37, 21 May 2024
NGC 6242 | |
---|---|
Observation data (J2000 epoch) | |
Right ascension | 16h 55m 30.7s[1] |
Declination | −39° 28′ 26″[1] |
Distance | 4.35 ± 0.53 kly (1.335 ± 0.163 kpc)[2] |
Apparent magnitude (V) | 6.4[3] |
Apparent dimensions (V) | 9′[3] |
Physical characteristics | |
Estimated age | 77.6[2] Myr |
Other designations | NGC 6242, Cr 317[4] |
Associations | |
Constellation | Scorpius |
NGC 6242 is an open cluster of stars in the southern constellation Scorpius. It can be viewed with binoculars or a telescope at about 1.5° to the south-southeast of the double star Mu Scorpii.[3] This cluster was discovered by French astronomer Nicolas-Louis de Lacaille in 1752 from South Africa.[5] It is located at a distance of approximately 4,350 ly (1,335 pc) from the Sun,[2] just to the north of the Sco OB 1 association.[6] The cluster has an estimated age of 77.6 million years.[2]
A microquasar with the designation GRO J1655-40 is located in the vicinity of NGC 6242 and is moving away from the cluster with a runaway space velocity of 112±18 km/s. It may have originated in the cluster during a supernova explosion ~2.2×105 year ago.[7]
References
- ^ a b Tarricq, Y.; et al. (March 2021). "3D kinematics and age distribution of the open cluster population". Astronomy & Astrophysics. 647. id. A19. arXiv:2012.04017. Bibcode:2021A&A...647A..19T. doi:10.1051/0004-6361/202039388.
- ^ a b c d Spina, L.; et al. (2021). "The GALAH survey: Tracing the Galactic disc with open clusters". Monthly Notices of the Royal Astronomical Society. 503 (3): 3279. arXiv:2011.02533. Bibcode:2021MNRAS.503.3279S. doi:10.1093/mnras/stab471.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b c Crossen, Craig; Rhemann, Gerald (2012). Sky Vistas, Astronomy for Binoculars and Richest-Field Telescopes. Springer Vienna. p. 52. ISBN 9783709106266.
- ^ "NGC 6242". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2007-04-24.
- ^ Jones, K. G. (March 1969). "The search for the nebulae - VI". Journal of the British Astronomical Association. 79: 213–222. Bibcode:1969JBAA...79..213J.
- ^ Sana, H.; et al. (August 2006). "An XMM-Newton view of the young open cluster NGC 6231. I. The catalogue". Astronomy and Astrophysics. 454 (3): 1047–1063. arXiv:astro-ph/0603783. Bibcode:2006A&A...454.1047S. doi:10.1051/0004-6361:20053224.
- ^ Combi, J. A.; et al. (May 2007). "New evidence on the origin of the microquasar GRO J1655-40". Astronomy and Astrophysics. 467 (2): 597–602. arXiv:astro-ph/0703674. Bibcode:2007A&A...467..597C. doi:10.1051/0004-6361:20077156.
External links
- Media related to NGC 6242 at Wikimedia Commons
- NGC 6242 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS – NGC 6242