Sh2-228

Sh2-228
Regione H II
Sh2-228
Dati osservativi
(epoca J2000)
CostellazioneAuriga
Ascensione retta05h 13m 26s[1]
Declinazione+37° 27′ 01″[1]
Coordinate galattichel = 169,2; b = -00,9[1]
Distanza11410[2] a.l.
(3500[2] pc)
Magnitudine apparente (V)-
Dimensione apparente (V)8' x 8'
Caratteristiche fisiche
TipoRegione H II
Classe3 2 3[3]
Caratteristiche rilevantiAvedisova 1729
Altre designazioni
LBN 784; Min 2-58[1]
Mappa di localizzazione
Sh2-228
Categoria di regioni H II

Sh2-228 è una nebulosa a emissione visibile nella costellazione dell'Auriga.

Si individua all'interno del grande pentagono che costituisce la costellazione, circa 1° a sud della stella μ Aurigae; il periodo più indicato per la sua osservazione nel cielo serale ricade fra i mesi di ottobre e marzo ed è notevolmente facilitata per osservatori posti nelle regioni dell'emisfero boreale terrestre.

Sh2-228 è una regione H II situata sul Braccio di Perseo a circa 3500 parsec (circa 11410 anni luce) di distanza;[2] possiede una forma asimmetrica ed è situata vicino alla grande associazione Auriga OB1. Si tratta di una vasta regione in cui è attiva la formazione stellare, come è ben evidenziato dalla presenza, al suo interno, di un giovane ammasso aperto piuttosto compatto noto come CC 01, formato da alcune stelle blu intrinsecamente molto luminose accompagnate da una numerosa popolazione di stelle più deboli; la loro età è stimata attorno a 1-2 milioni di anni al massimo e rappresentano una generazione di stelle successiva rispetto alle stelle circostanti, che mostrano invece un'età di circa 5-6 milioni di anni. La massa totale dell'ammasso si aggira sulle 1800 M.[2] Nel Catalogo Avedisova la nebulosa è associata anche ad alcune sorgenti di onde radio.[4]

Da notare infine che studi basati sulle emissioni alle onde radio hanno fornito per Sh2-228 una distanza nettamente superiore, attorno ai 7900 parsec (oltre 25000 anni luce).[5]

Note

  1. ^ a b c d Simbad Query Result, su simbad.u-strasbg.fr. URL consultato il 25 aprile 2013.
  2. ^ a b c d Borissova, J.; Pessev, P.; Ivanov, V. D.; Saviane, I.; Kurtev, R.; Ivanov, G. R., Discovery of new Milky Way star cluster candidates in the 2MASS Point Source Catalog. II. Physical properties of the star cluster CC 01, in Astronomy and Astrophysics, vol. 411, novembre 2003, pp. 83-90, DOI:10.1051/0004-6361:20034009. URL consultato il 25 aprile 2013.
  3. ^ Sharpless, Stewart, A Catalogue of H II Regions., in Astrophysical Journal Supplement, vol. 4, dicembre 1959, p. 257, DOI:10.1086/190049. URL consultato il 25 aprile 2013.
  4. ^ Avedisova, V. S., A Catalog of Star-Forming Regions in the Galaxy, in Astronomy Reports, vol. 46, n. 3, marzo 2002, pp. 193-205, DOI:10.1134/1.1463097. URL consultato il 25 aprile 2013.
  5. ^ Paladini, R.; Burigana, C.; Davies, R. D.; Maino, D.; Bersanelli, M.; Cappellini, B.; Platania, P.; Smoot, G., A radio catalog of Galactic HII regions for applications from decimeter to millimeter wavelengths, in Astronomy and Astrophysics, vol. 397, gennaio 2003, pp. 213-226, DOI:10.1051/0004-6361:20021466. URL consultato il 25 aprile 2013.

Bibliografia

  • Tirion, Rappaport, Lovi, Uranometria 2000.0 - Volume I - The Northern Hemisphere to -6°, Richmond, Virginia, USA, Willmann-Bell, inc., 1987, ISBN 0-943396-14-X.
  • Tirion, Sinnott, Sky Atlas 2000.0 - Second Edition, Cambridge, USA, Cambridge University Press, 1998, ISBN 0-933346-90-5.

Voci correlate

Collegamenti esterni

  • Sky-Map.org - Sharpless Catalogue (from 221 to 230) [collegamento interrotto], su galaxymap.org.
  Portale Oggetti del profondo cielo: accedi alle voci di Wikipedia che trattano di oggetti non stellari

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