Strooan y Tideyr

Ta Strooan y Tideyr (Baarle: [Sagittarius Stream] Error: {{Lang}}: text has italic markup (help)) çheet er strughtoor ard-hroggalagh liauyr dy rollageyn ta filley mygeayrt Raad Mooar Gorree ayns cruinlagh ta begnagh goll tessen ny poullyn galactagh. T'eh jeant jeh rollageyn va raipit dy tidee veih Co-rollageys Crivassanagh Eelipsagh y Tideyr, myr eiyrtys er obbraghey yn vestey jeh rish Raad Mooar Gorree harrish billoonyn dy vleeantyn.

Va'n strooan rollageagh shoh currit roish lesh Donald Lynden-Bell 'sy vlein 1995 erreish da ren eh oltscarrey rheynn ny dhossanyn bluckanagh ayns Raad Mooar Gorree.^[1] Chur Newberg as e choheshaghtee (2002)^[2] as Majewski as e choheshaghtee (2003)^[3] enney er y strughtoor hene lesh fysseree veih ny towshanyn 2MASS as SDSS. 'Sy vlein 2006, ren Belokurov as e cho-obbreeyn^[4] feddyn magh dy row daa vanglane ec Strooan y Tideyr.

Tra va'n nhee shannayragh mynyiarrit veih e cheilley car yn eddyr-obbraghey, chur eh leaystaghyn (cosoylagh rish sheean-tonnyn) trooid strughtoor laue chaslagh Raad Mooar Gorree. Ta bree ny leaystaghyn shen ry-akin jiu myr bratyn çhiu as goan jeh rheynnyn rollageagh erskyn as fo Corys ny Greiney. Jiu, ta soiaghey Strooan y Tideyr conastagh rish ny brattyn baghtallagh^[5] cur rish y smooinaght dy vel Co-hollys Crivassanagh Eelipsagh y Tideyr kyndagh lesh y vrishey stiagh shen.

Jeeagh er neesht

Rolley strooanyn rollageagh

Imraaghyn

↑ Lynden-Bell, R. M.; Lynden-Bell, D. (Jerrey Souree 1995). "Ghostly streams from the formation of the Galaxy's halo". Monthly Notices of the Royal Astronomical Society. 275 (2): 429–442. Bibcode:1995MNRAS.275..429L. doi:10.1093/mnras/275.2.429.
↑ Newberg, Heidi Jo; et al. (Averil 2002). "The Ghost of Sagittarius and Lumps in the Halo of the Milky Way". The Astrophysical Journal. 569 (1): 245–274. arXiv:astro-ph/0111095. Bibcode:2002ApJ...569..245N. doi:10.1086/338983. S2CID 16909562.
↑ Majewski, Steven R.; et al. (Nollick 2003). "A Two Micron All Sky Survey View of the Sagittarius Dwarf Galaxy. I. Morphology of the Sagittarius Core and Tidal Arms". The Astrophysical Journal. 599 (2): 1082–1115. arXiv:astro-ph/0304198. Bibcode:2003ApJ...599.1082M. doi:10.1086/379504. S2CID 2387702.
↑ Belokurov, V.; et al. (Boaldyn 2006). "The Field of Streams: Sagittarius and Its Siblings". The Astrophysical Journal. 642 (2): L137–L140. arXiv:astro-ph/0605025. Bibcode:2006ApJ...642L.137B. doi:10.1086/504797. S2CID 1774643.
↑ Yanny, Brian; Gardner, Susan (Mean Fouyir 2013). "The Stellar Number Density Distribution in the Local Solar Neighborhood is North-South Asymmetric". The Astrophysical Journal. 777 (2): 91. arXiv:1309.2300. Bibcode:2013ApJ...777...91Y. doi:10.1088/0004-637X/777/2/91. S2CID 118314811.

Kianglaghyn magh

Deriving The Shape Of The Galactic Stellar Disc (SkyNightly) 17 Mayrnt 2006
Deriving the shape of the Galactic stellar disc, cur-magh naight A&A, 16 Mayrnt 2006

[LB2-1] Lynden-Bell, R. M.; Lynden-Bell, D. (Jerrey Souree 1995). "Ghostly streams from the formation of the Galaxy's halo". Monthly Notices of the Royal Astronomical Society. 275 (2): 429–442. Bibcode:1995MNRAS.275..429L. doi:10.1093/mnras/275.2.429.

[Discovery1-2] Newberg, Heidi Jo; et al. (Averil 2002). "The Ghost of Sagittarius and Lumps in the Halo of the Milky Way". The Astrophysical Journal. 569 (1): 245–274. arXiv:astro-ph/0111095. Bibcode:2002ApJ...569..245N. doi:10.1086/338983. S2CID 16909562.

[Discover21-3] Majewski, Steven R.; et al. (Nollick 2003). "A Two Micron All Sky Survey View of the Sagittarius Dwarf Galaxy. I. Morphology of the Sagittarius Core and Tidal Arms". The Astrophysical Journal. 599 (2): 1082–1115. arXiv:astro-ph/0304198. Bibcode:2003ApJ...599.1082M. doi:10.1086/379504. S2CID 2387702.

[Streams-4] Belokurov, V.; et al. (Boaldyn 2006). "The Field of Streams: Sagittarius and Its Siblings". The Astrophysical Journal. 642 (2): L137–L140. arXiv:astro-ph/0605025. Bibcode:2006ApJ...642L.137B. doi:10.1086/504797. S2CID 1774643.

[Yanny2013-5] Yanny, Brian; Gardner, Susan (Mean Fouyir 2013). "The Stellar Number Density Distribution in the Local Solar Neighborhood is North-South Asymmetric". The Astrophysical Journal. 777 (2): 91. arXiv:1309.2300. Bibcode:2013ApJ...777...91Y. doi:10.1088/0004-637X/777/2/91. S2CID 118314811.

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