Search: onr:"swepub:oai:DiVA.org:su-36185" > Deep V and K band p...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 01701naa a2200265 4500 | |
001 | oai:DiVA.org:su-36185 | |
003 | SwePub | |
008 | 100122s2009 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-361852 URI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a pop2 swepub-contenttype |
072 | 7 | a kon2 swepub-publicationtype |
100 | 1 | a Micheva, Genovevau Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)gemi0323 |
245 | 1 0 | a Deep V and K band photometry of the host galaxy of Haro 11 |
264 | 1 | c 2009 |
338 | a print2 rdacarrier | |
520 | a Previous studies of the host galaxy of Haro 11 have suggested an extreme red color of V-K=4.2+-0.8 which cannot be reconciled with any normal stellar population of reasonable metallicity. We present the deepest V and K band data to date of the blue compact galaxy (BCG) Haro 11 and derive a new V-K color for the host. Our new data suggest a much more modest value of V-K=2.3+-0.2, which is in the same range as V-K colors measured for several other BCGs. The new Haro 11 color is not abnormally red and can be attributed to an old metal-poor stellar population with a Salpeter initial mass function. | |
653 | a Astrophysics - Cosmology and Extragalactic Astrophysics | |
700 | 1 | a Zackrisson, Eriku Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)erza6638 |
700 | 1 | a Östlin, Göranu Stockholms universitet,Institutionen för astronomi4 aut0 (Swepub:su)ostlin |
700 | 1 | a Bergvall, Nils4 aut |
710 | 2 | a Stockholms universitetb Institutionen för astronomi4 org |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-36185 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.