Dwingeloo 1
![Sky map](http://upload.wikimedia.org/wikipedia/commons/thumb/e/e4/Jupiter_and_moon.png/20px-Jupiter_and_moon.png)
Dwingeloo 1 | |
---|---|
Group or cluster | IC 342/Maffei |
Apparent magnitude (V) | 13.08 (V-band)[4] |
Characteristics | |
Type | SB(s)cd[1] |
Apparent size (V) | 4.2′ × 0.34′[1] |
Other designations | |
LEDA 100170, CAS 2[1] |
Dwingeloo 1 is a
Dwingeloo 1 has two smaller satellite galaxies – Dwingeloo 2 and MB 3 – and is a member of the IC 342/Maffei Group of galaxies.
Discovery
The Dwingeloo 1 galaxy was discovered in 1994 by the Dwingeloo Obscured Galaxy Survey (DOGS) using the Dwingeloo Radio Observatory, which searched for neutral hydrogen (HI) radio emissions at the wavelength of 21 cm from objects in the Zone of Avoidance. In this zone gas and dust in the disk of the Milky Way galaxy block the light from the galaxies lying behind it.[5]
The galaxy was, however, first noted as an unremarkable feature on
Dwingeloo 1 was eventually named after the 25m radio telescope in the Netherlands that was used in the DOGS survey and first detected it.[5]
Distance and group membership
Dwingeloo 1 is a highly obscured galaxy, which makes distance determination a difficult problem. The initial estimate, made soon after the discovery and based on the Tully–Fisher relation, was about 3 Mpc.[5] Later, this value was slightly increased to 3.5–4 Mpc.[7]
In 1999 another estimate was published, claiming a distance of more than 5 Mpc. It was based on the infrared Tully–Fisher relation.[8] As of 2011, the distance to Dwingeloo 1 is thought to be approximately 3 Mpc, based on its likely membership in the IC 342/Maffei group.[3]
Dwingeloo 1 has two smaller satellite galaxies. The first one, Dwingeloo 2, is an irregular galaxy,[2] and the second, MB 3, is likely a dwarf spheroidal galaxy.
Properties
After the discovery Dwingeloo 1 was classified as a barred spiral galaxy.[5] It has a central bar and two distinct spiral arms that begin at the ends of the bar at nearly right angles and wind counterclockwise. The length of the arms is up to 180°.[5] The disk of the galaxy is inclined with respect to the observer, with the inclination angle being 50°. The galaxy recedes from the Milky Way at a speed of about 256 km/s.[7]
The visible radius of Dwingeloo 1 is approximately 4.2', which at the distance of 3 Mpc corresponds to about 4 kpc. The neutral hydrogen is detected as far as 6 kpc (7.5') from the center. The total mass of the galaxy is about 1/4 that of the Milky Way out to the measured distance of 6 kpc or about 31 billion Solar masses.[2]
The distribution of the neutral hydrogen in Dwingeloo 1 is typical for barred spiral galaxies—it is rather flat with a minimum in the center or along the bar.
In its overall size and mass, the galaxy is comparable to Triangulum Galaxy.[5]
See also
References
- ^ a b c d e f "NASA/IPAC Extragalactic Database". Results for Dwingeloo 1. Retrieved 2006-11-21.
- ^ Bibcode:1996A&A...309..687B.
- ^ S2CID 119385141.
- S2CID 119907629.
- ^ S2CID 4242688.
- ^ Bibcode:1995A&A...293L..33H.
- ^ .
- S2CID 15619332.
- .
External links
- "NAME Cas 2". SIMBAD. Centre de données astronomiques de Strasbourg.
- Nemiroff, R.; Bonnell, J., eds. (9 January 2000). "Galaxy Dwingeloo 1 Emerges". Astronomy Picture of the Day. NASA.