Zobrazeno 1 - 9
of 9
pro vyhledávání: '"C. J. Grillmair"'
Autor:
C. J. Grillmair
Publikováno v:
The Astrophysical Journal. 651:L29-L32
We report on the detection in Sloan Digital Sky Survey data of at least three, roughly parallel components in a 65 degree-long stellar stream complex previously identified with the Anticenter or Monoceros Ring. The three-stream complex varies in widt
Autor:
C. J. Grillmair, Odysseas Dionatos
Publikováno v:
The Astrophysical Journal. 641:L37-L39
Using Data Release 4 of the Sloan Digital Sky Survey, we have applied an optimal contrast, matched filter technique to trace the trailing tidal tail of the globular cluster Palomar 5 to a distance of 18.5 degrees from the center of the cluster. This
Autor:
G. Fiorentino, A. Monachesi, S. Trager, T. Lauer, A. Saha, K. Mighell, W. L. Freedman, A. Dressler, C. J. Grillmair, E. Tolstoy, Joyce Ann Guzik, Paul A. Bradley
Publikováno v:
STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION, 216-220
STARTPAGE=216;ENDPAGE=220;TITLE=STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION
STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION, 1170, 216-220
STARTPAGE=216;ENDPAGE=220;TITLE=STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION
STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION, 1170, 216-220
We observed two fields near M32 with the ACS/HRC on board the Hubble Space Telescope, located at distances of about 1.8' and 5.4' (hereafter F1 and F2, respectively) from the center of M32. To obtain a very detailed and deep color-magnitude diagram (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::609506dccbb59246c5025bbb54565c55
http://arxiv.org/abs/0909.0202
http://arxiv.org/abs/0909.0202
Autor:
J. R. Houck, T. L. Roellig, J. van Cleve, W. J. Forrest, T. Herter, C. R. Lawrence, K. Matthews, H. J. Reitsema, B. T. Soifer, D. M. Watson, D. Weedman, M. Huisjen, J. Troeltzsch, D. J. Barry, J. Bernard‐Salas, C. E. Blacken, B. R. Brandl, V. Charmandaris, D. Devost, G. E. Gull, P. Hall, C. P. Henderson, S. J. U. Higdon, B. E. Pirger, J. Schoenwald, G. C. Sloan, K. I. Uchida, P. N. Appleton, L. Armus, M. J. Burgdorf, S. B. Fajardo‐Acosta, C. J. Grillmair, J. G. Ingalls, P. W. Morris, H. I. Teplitz
The Infrared Spectrograph (IRS) is one of three science instruments on the Spitzer Space Telescope. The IRS comprises four separate spectrograph modules covering the wavelength range from 5.3 to 38micron with spectral resolutions, R \~90 and 600, and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96b3fe77b28395d10897c9e7a0f04555
http://arxiv.org/abs/astro-ph/0406167
http://arxiv.org/abs/astro-ph/0406167
Autor:
L. Armus, V. Charmandaris, H. W. W. Spoon, J. R. Houck, B. T. Soifer, B. R. Brandl, P. N. Appleton, H. I. Teplitz, S. J. U. Higdon, D. W. Weedman, D. Devost, P. W. Morris, K. I. Uchida, J. van Cleve, D. J. Barry, G. C. Sloan, C. J. Grillmair, M. J. Burgdorf, S. B. Fajardo‐Acosta, J. G. Ingalls, J. Higdon, L. Hao, J. Bernard‐Salas, T. Herter, J. Troeltzsch, B. Unruh, M. Winghart
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2004, 154, pp.178-183
The Astrophysical Journal, 2004, 154, pp.178-183
We present spectra taken with the Infrared Spectrograph on Spitzer covering the 5-38micron region of three Ultraluminous Infrared Galaxies (ULIRGs): Mrk 1014 (z=0.163), and Mrk 463 (z=0.051), and UGC 5101 (z=0.039). The continua of UGC 5101 and Mrk 4
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b72ff3fdf56f8949360e6ff2674eed47
Autor:
J. R. Hargis, S. Albers, D. Crnojević, D. J. Sand, D. R. Weisz, J. L. Carlin, K. Spekkens, B. Willman, A. H. G. Peter, C. J. Grillmair, A. E. Dolphin
Publikováno v:
Astrophysical Journal; Jan2020, Vol. 888 Issue 1, p1-1, 1p
Autor:
C. J. Pritchet, C. J. Grillmair
Publikováno v:
Publications of the Astronomical Society of the Pacific. 96:349
High-sensitivity spectrophotometry has been obtained over the spectral range 5000-6000 A for the planetary nebulae NGC 6210, NGC 7027, and IC 351 and for the bipolar nebula AFGL 2688. The observations of NGC 7027 show an emission feature at 5624 A wh
Autor:
R. G. Carlberg, C. J. Grillmair
Publikováno v:
Astrophysical Journal; 10/20/2016, Vol. 830 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal Letters; 10/10/2015, Vol. 812 Issue 1, p1-1, 1p