|
| |
| | APOD Search Results for "galaxy" |
 | | NGC 7331 is interesting in part because it is thought to be so similar to the Milky Way. | | | The resulting turbulent environment is fed by supernova explosions as the cosmic detonations spew out material and trigger further star formation. | | | First, the galaxy's star distribution merits a formal classification of dwarf |
|
http://antwrp.gsfc.nasa.gov/cgi-bin/apod/apod_search?galaxy
|
|
| |
| | Neutral hydrogen studies |
| | One of these, NGC 4559, shows a strongly kinematically lopsided disk and the presence of anomalous HI as NGC 2403. | | | The shapes of the HI and optical rotation curves have been compared with the distribution of luminous matter as inferred from photometric profiles. | | | Very deep (16x12 hours integration) HI observations with the upgraded WSRT are planned. |
|
http://www.bo.astro.it/report01/node34.html
|
|
| |
| | 2MASS Atlas Image Gallery |
| | In the near-IR the very prominent and patchy dust lanes seen in the optical image are far less obvious; the overall light distribution in the near-IR is smoother, even though the galaxy disk is significantly inclined. | | | conclude that if seen face-on, NGC 891 would be optically thin, and that from its estimated dust mass and extinction law, this galaxy is indeed very much like our own Milky Way. | | | Compare the 2MASS view of this system with that obtained by the Hubble Space Telescope in the optical. |
|
http://www.ipac.caltech.edu/2mass/gallery/images_galaxies.html
|
|
| |
| | Hubble Space Telescope, Thumbnail Views page 6 |
| | NGC 2346, Butterfly Nebula : The nebula is about 2,000 light-years from Earth in the direction of the constellation Monoceros. | | | NGC 3372, Keyhole Nebula : Details of a mysterious, complex structure within the Carina Nebula are revealed by this image of the "Keyhole Nebula." The pic is dominated by a large, almost circular feature, which is part of the keyhole. | | | The clumps that form the comet heads all seem to be located at a similar distance from the star; a fact that will be important in developing a theory of why the clumps formed. |
|
http://www.laughtergenealogy.com/bin/hubble/thumbs06.html
|
|
| |
| | List of Nice Objects |
| | The final group of objects is definitely candidates for the largest CCD chips and digital cameras. | | | NGC 2174 06 09.7 20 30 40x30 ? | | | NGC 2024 05 41.9 -01 50 20x20 ? |
|
http://www.mailbag.com/users/ragreiner/objects.html
|
|
| |
| | NGC 2976, Spiral Galaxy |
| | This is another dwarf system with a computed diameter of about 7,000 light years. | | | The large spiral NGC 2403 in Camelopardalis also appears to be a dynamical member of this group. | | | This is another odd galaxy, usually classed as a spiral of type Sd although very little evidence of spiral structure appears on photographs. |
|
http://www.kopernik.org/images/archive/n2976.htm
|
|
| |
| | NGC 2403 |
| | In the SAC 110 best NGC object list. | | | 37 in the RASC Finest NGC Objects list. | | | One supernova has been recorded in this galaxy so far: Supernova 1954J, which was discovered by Zwicky (PASP 84, 844) on October 24, 1954. |
|
http://astronomy.nju.edu.cn/astron/messier/n2403.html
|
|
| |
| | NGC 2403, Spiral Galaxy |
| | There are also a number of supernova remnants. | | | NGC 2403 was the first galaxy beyond the Local Group in which Cepheid variables were found. | | | Over 100 H-II star forming regions, many of them irregular in shape, are known in NGC 2403. |
|
http://www.kopernik.org/images/archive/n2403.htm
|
|
| |
| | Comparing Correlation Dimensions and Capacity Dimensions |
| | When the contours are drawn around NGC 2403 for various values of magnitudes, they break into many small contours creating a distribution of points at greater distances. | | | From our discussion, we would expect the difference between the averages of the correlation dimension and the capacity dimension to be positive but the difference turns out to be a negative number. | | | From our discussion, we would expect the above mentioned difference to be negative but it turns out to be a positive number, making the average correlation dimension higher than the average capacity dimension. |
|
http://www.physics.unlv.edu/~thanki/thesis/node22.html
|
|
| |
| | S105 Student Work |
| | The Flame Nebula, also known as the Burning Tree Nebula (and as NGC 2024) is imaged in three filters, a red filter (R), an H-alpha filter, and a [S II] filter. | | | The H-alpha filter shows us the many striking regions of star formation found in NGC 2403. | | | This spiral galaxy is member of the local group of galaxies, which also includes our own Milky Way Galaxy and the Andromeda Galaxy (M31). |
|
http://enif.astro.indiana.edu/s105_work.htm
|
|
| |
| | No Title |
| | NGC 2403 is a luminous spiral with a high rate of star formation and it represents one of the few cases of disk galaxies with diffuse X-ray emission known to-date. | | | K) is well separated from the numerous bright point sources. | | | This emerging picture of NGC 2403 as an "effervescent" spiral galaxy is likely to become a prototype for the entire class of late-type spirals with active star formation. |
|
http://asc.harvard.edu/symposium_2001/NG/89clean/89clean.html
|
|
| |
| | Spiral Galaxy NGC 2403 - Wikipedia, the free encyclopedia |
| | Spiral Galaxy NGC 2403 (also known as NGC 2403) is a spiral galaxy in the Camelopardalis constellation. | | | This page was last modified 02:32, 16 Jan 2005. | | | NGC 2403 is a type Sc spiral, an outlying member of the M81 group, and is approximately 11 million light years distant. |
|
http://en.wikipedia.org/wiki/NGC_2403
|
|
| |
| | Other known galaxies |
| | Images will not be available for d/l due to server space limitations, however original format is available on demand. | | | Note: Data has been compiled according to the Messier Objects Catalogue (M) and New General Catalogue (NGC) | | | M75 Globular Cluster NGC 6864 (class I) in Sagittarius |
|
http://pages.infinit.net/bluhaze/Glxs2.htm
|
|
| |
| | Best of AOP: NGC 2403 |
| | This galaxy extends well beyond this field of view- note the very blue arms reaching towards the edges of the frame. | | | Would you like to take images like this? | | | This galaxy is estimated to be around 12 million light years away. |
|
http://www.noao.edu/noao/pio/pop/advanced/observers/n2403.html
|
|
| |
| | NGC 2403 |
| | All files associated with The Constellations Web Page are | | | Having verified that you're in the right location, now put 42 and 43 at the northwest corner of your field of vision. | | | The galaxy is in the same field as 42 and 43 Cam. |
|
http://www.dibonsmith.com/ngc2403.htm
|
|
| |
| | Galaxy NGC 2403 and supernova 2004dj |
| | It was easy to identify from a CDD-picture. | | | Supernova 2004dj (arrow) was the reason why I observed this galaxy. | | | NGC 2403 was difficult to see because of bright background sky. |
|
http://deepsky.iwarp.com/havaintongc2403.htm
|
|
| |
| | NGC2403 |
| | This beautiful galaxy is one of the nearest outside of our local group and is probably a member of the M81/M82 Group. |
|
http://schmidling.netfirms.com/ngc2403.htm
|
|
| |
| | Summary of sequence number 600148 |
| | In particular, the presence or absence of a hot counterpart of the HI halo will contribute new crucial information for understanding the evolution of NGC 2403 in particular and similar galaxies in general. | | | Deep HI observations have revealed numerous expanding superbubbles in the disk and an extensive HI halo with large and peculiar kinematics. | | | The aims of this proposal are i) the study of X-ray emission from the superbubbles and ii) the search for a hot diffuse emission from the halo. |
|
http://asc.harvard.edu/cgi-gen/mp/target.cgi?600148
|
|
| |
| | [No title] |
| | A Chandra observation of the neutron star X-ray transient and eclipsing binary MXB 1659-29 in quiescence | | | X-ray Source Population in the Elliptical Galaxy NGC 720 with Chandra | | | Prospects for the Determination of H_0 Through Observation of Multiply Imaged Supernovae in Galaxy Cluster Fields |
|
http://space.mit.edu/pubs2003.html
|
|
| |
| | Photo Index |
| | NGC 2244 Rosette Nebula in Monoceros with detail of Bok globules | | | NGC 3389 Spiral Galaxy in Leo (large scale)... | | | NGC 7009 Saturn Nebula in Aquarius (Film)...(CCD Image) |
|
http://schmidling.netfirms.com/phoindex.htm
|
|
| |
| | Galaxies |
| | NGC 4214 - An irregular Dwarf/Wolf Rayet galaxy in Canes Venatici | | | NGC 3239 - An irregular interacting galaxy in Leo | | | NGC 5987 - A nearly edge on small galaxy in Draco |
|
http://www.astrophotos.net/pages/galaxies.htm
|
|
| |
| | Spriral and lecticular galaxies |
| | Central region of the Active Galaxy NGC 1068 | | | NGC 4321, M-100 (HST) Spiral in Virgo Cluster | | | Stellar population I and II 342 at 2.8cm radio emission |
|
http://outreach.as.utexas.edu/eso/slides/wc.html
|
|
|
