Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Rokas Naujalis"'
Publikováno v:
Proceedings of the International Astronomical Union. 14:131-134
We performed a new integrated photometry in six passbands on HST M31 PHAT survey mosaics of 1181 star clusters spread over a large range of radial distance. Due to strongly varying background we interactively determined its level based on image and g
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::70aafb93983874b9738c5cee78bde003
https://doi.org/10.1017/s1743921319007300
https://doi.org/10.1017/s1743921319007300
Autor:
Rokas Naujalis
Star Clusters in Galaxies. Multicolour HST photometry
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::213e849d1493674a890cb2c8b63d79d2
https://doi.org/10.15388/vu.thesis.113
https://doi.org/10.15388/vu.thesis.113
Leo A is an isolated gas-rich dwarf irregular galaxy of low stellar mass and metallicity residing at the outskirts of the Local Group. Ages of the stellar populations in Leo A range from $\sim$10 Myr to $\sim$10 Gyr. So far, only one star cluster has
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::20e4036ca9fe4a42986717d793af3e82
Publikováno v:
Astronomy & Astrophysics. 614:A144
Context. Leo A is an isolated gas-rich dwarf irregular galaxy of low stellar mass and metallicity residing at the outskirts of the Local Group. Ages of the stellar populations in Leo A range from ~10 Myr to ~10 Gyr. A large stellar halo (up to the de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::90dfb3c5e1b99101976b160a32f784b9
https://doi.org/10.1051/0004-6361/201731840
https://doi.org/10.1051/0004-6361/201731840
Recent analytical and numerical models show that AGN outflows and jets create ISM pressure in the host galaxy that is several orders of magnitude larger than in quiescent systems. This pressure increase can confine and compress molecular gas, thus ac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d7bc196fb9b29754350d629143ecd9b
http://arxiv.org/abs/1405.7516
http://arxiv.org/abs/1405.7516