Zobrazeno 1 - 10
of 101
pro vyhledávání: '"PELETIER, RF"'
Publikováno v:
The Astronomical Journal, 100(4), 1091-1142. IOP PUBLISHING LTD
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::affa7acac1f93e3ba3e46a5f91d6aa31
https://ora.ox.ac.uk/objects/uuid:1cdda4b2-4b26-4e1d-80d8-1499e47d860a
https://ora.ox.ac.uk/objects/uuid:1cdda4b2-4b26-4e1d-80d8-1499e47d860a
Autor:
Jeong, H, Yi, SK, Bureau, M, Davies, RL, Bacon, R, Cappellari, M, de Zeeuw, PT, Emsellem, E, Falcon-Barroso, J, Krajnovic, D, Kuntschner, H, McDermid, RM, Peletier, RF, Sarzi, M, van den Bosch, RCE, van de Ven, G
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 423(2), 1921-1939. Oxford University Press
The unexpected rising flux of early-type galaxies at decreasing ultraviolet (UV) wavelengths is a long-standing mystery. One important observational constraint is the correlation between UV-optical colours and Mg2 line strengths found by Burstein et
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::149878c8d5f2c36cec02ac48a8e4a72a
https://research.rug.nl/en/publications/007b03e9-e2e3-4fb7-842d-fedf26b91537
https://research.rug.nl/en/publications/007b03e9-e2e3-4fb7-842d-fedf26b91537
Autor:
Bureau, M, Jeong, H, Yi, SK, Schawinski, K, Houghton, RCW, Davies, RL, Bacon, R, Cappellari, M, Zeeuw, PTD, Emsellem, E, Falcon-Barroso, J, Krajnovic, D, Kuntschner, H, McDermid, RM, Peletier, RF, Sarzi, M, Sohn, YJ, Thomas, D, Bosch, RCEVD, Ven, GVD
Using far (FUV) and near (NUV) ultraviolet photometry from guest investigator programmes on the Galaxy Evolution Explorer (GALEX) satellite, optical photometry from the MDM Observatory and optical integral-field spectroscopy from SAURON, we explore t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::de3f51ac79593aa6199b3ca6a5ffdf13
http://arxiv.org/abs/1102.0957
http://arxiv.org/abs/1102.0957
Autor:
Carter, D, Goudfrooij, P, Mobasher, B, Ferguson, HC, Puzia, TH, Aguerri, AL, Balcells, M, Batcheldor, D, Bridges, TJ, Davies, JI, Erwin, P, Graham, AW, Guzmán, R, Hammer, D, Hornschemeier, A, Hoyos, C, Hudson, MJ, Huxor, A, Jogee, S, Komiyama, Y, Lotz, J, Lucey, JR, Marzke, RO, Merritt, D, Miller, BW, Miller, NA, Mouhcine, M, Okamura, S, Peletier, RF, Phillipps, S, Poggianti, BM, Sharples, RM, Smith, RJ, Trentham, N, Tully, RB, Valentijn, E, Kleijn, GV
We describe the HST ACS Coma cluster Treasury survey, a deep two-passband imaging survey of one of the nearest rich clusters of galaxies, the Coma cluster (Abell 1656). The survey was designed to cover an area of 740 square arcmin in regions of diffe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4370eecbd09920122a3d17ed030b0320
http://arxiv.org/abs/0801.3745
http://arxiv.org/abs/0801.3745
Autor:
van Woerden, H, Wakker, BP, Peletier, RF, Schwarz, UJ, KraanKorteweg, RC, Henning, PA, Andernach, H
Publikováno v:
MAPPING THE HIDDEN UNIVERSE: THE UNIVERSE BEHIND THE MILKY WAY-THE UNIVERSE IN HI, PROCEEDINGS, 407-417
STARTPAGE=407;ENDPAGE=417;TITLE=MAPPING THE HIDDEN UNIVERSE: THE UNIVERSE BEHIND THE MILKY WAY-THE UNIVERSE IN HI, PROCEEDINGS
STARTPAGE=407;ENDPAGE=417;TITLE=MAPPING THE HIDDEN UNIVERSE: THE UNIVERSE BEHIND THE MILKY WAY-THE UNIVERSE IN HI, PROCEEDINGS
A review is given of distances of high-velocity clouds (HVCs) derived from absorption-line measurements, and of the metallicities of HVCs. Chain A definitely lies in the Galactic halo, between 2.5 and 7 kpc above the plane. The distance limits availa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::47fc5421f0f7fcbb3703097fac7aeada
https://research.rug.nl/en/publications/dedc54f6-1c2f-44c3-915d-73c0505d5e71
https://research.rug.nl/en/publications/dedc54f6-1c2f-44c3-915d-73c0505d5e71
Publikováno v:
STROMLO WORKSHOP ON HIGH-VELOCITY CLOUDS, 1-25
STARTPAGE=1;ENDPAGE=25;TITLE=STROMLO WORKSHOP ON HIGH-VELOCITY CLOUDS
STARTPAGE=1;ENDPAGE=25;TITLE=STROMLO WORKSHOP ON HIGH-VELOCITY CLOUDS
Distance and metallicity hold the key to our understanding of the physical properties and origins of HVCs. We review the problems and results of determinations of distance and metallicity based on the presence or absence, and strength, of appropriate
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::748fcece3d6a3c68b8f17711884fcc17
https://research.rug.nl/en/publications/44b6d802-8de3-4ef3-b513-7ed87f382669
https://research.rug.nl/en/publications/44b6d802-8de3-4ef3-b513-7ed87f382669
Publikováno v:
PLANETARY NEBULAE, 478-478
STARTPAGE=478;ENDPAGE=478;TITLE=PLANETARY NEBULAE
STARTPAGE=478;ENDPAGE=478;TITLE=PLANETARY NEBULAE
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::91425793bf2ac694f47dc8823c77f64b
https://research.rug.nl/en/publications/c27ac64c-6b36-4e2e-beea-339ca8d1c27b
https://research.rug.nl/en/publications/c27ac64c-6b36-4e2e-beea-339ca8d1c27b
Publikováno v:
Astrophysical Journal, 458(2), 533-536. IOP PUBLISHING LTD
We provide a new calibration of the metallicity dependence of the Mg-2 index in stellar systems. It is based on new isochrones by the Padova group and the latest stellar spectral libraries. Since the Mg-2 line is one of the strongest absorption lines
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::981606b6897d9cde746fecb8753d2cf6
https://research.rug.nl/en/publications/d0bfb359-c2f3-4817-9493-a8d635f5eb41
https://research.rug.nl/en/publications/d0bfb359-c2f3-4817-9493-a8d635f5eb41
Autor:
Wakker, BP, VanWoerden, H, Schwarz, UJ, Peletier, RF, Douglas, NG, Danly, L, DeBoer, KS, Blitz, L, Teuben, P
Publikováno v:
UNSOLVED PROBLEMS OF THE MILKY WAY, 605-606
STARTPAGE=605;ENDPAGE=606;TITLE=UNSOLVED PROBLEMS OF THE MILKY WAY
STARTPAGE=605;ENDPAGE=606;TITLE=UNSOLVED PROBLEMS OF THE MILKY WAY
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::eca8969dbc9785f9ef201d42bb9ee833
https://research.rug.nl/en/publications/cde79901-3e7e-4316-a4d5-49614e9081e7
https://research.rug.nl/en/publications/cde79901-3e7e-4316-a4d5-49614e9081e7
Publikováno v:
New light of Galaxy evolution, 29-33
STARTPAGE=29;ENDPAGE=33;TITLE=New light of Galaxy evolution
STARTPAGE=29;ENDPAGE=33;TITLE=New light of Galaxy evolution
For a sample of bright nearby early-type galaxies we have obtained surface photometry in bands ranging from U to K. Since the galaxies have inclinations larger than 50 degrees it is easy to separate bulges and disks. By measuring the colours in speci
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::4990214d8f3776b1590b1ae824130cb1
https://research.rug.nl/en/publications/667327d4-134b-49d4-9a36-01c6e2879ef8
https://research.rug.nl/en/publications/667327d4-134b-49d4-9a36-01c6e2879ef8