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[PDF] Top 20 Near infrared photometry and spectroscopy of the low Galactic latitude globular cluster 2MASS GC 03

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Near infrared photometry and spectroscopy of the low Galactic latitude globular cluster 2MASS GC 03

Near infrared photometry and spectroscopy of the low Galactic latitude globular cluster 2MASS GC 03

... from the Programa de Astronom´ıa del DRI Folio 32130012 and CONICYT-Chile grants FONDECYT Postdoctoral Fellowship ...SRA and CMB were supported by the Fondecyt project number 3140605 ... See full document

10

Near infrared photometry of globular clusters towards the Galactic bulge: Observations and photometric metallicity indicators

Near infrared photometry of globular clusters towards the Galactic bulge: Observations and photometric metallicity indicators

... 6401 and NGC 6558, our photometric values are ∼ ...on the RGB slope, so the uncertainties are relatively ...sparse and projected on the Galactic bulge, their TRGB magnitudes ... See full document

29

The next generation virgo cluster survey infrared (NGVS IR)  I  A new near ultraviolet, optical, and near infrared globular cluster selection tool

The next generation virgo cluster survey infrared (NGVS IR) I A new near ultraviolet, optical, and near infrared globular cluster selection tool

... 10 and 30 pc (Has¸egan et ...are the remnant nuclei of dwarf galaxies that were stripped by interactions ...erates of multiple clusters that merged early in their lifetimes during violent ... See full document

23

Structure and kinematics of Type II Cepheids in the Galactic bulge based on near infrared VVV data

Structure and kinematics of Type II Cepheids in the Galactic bulge based on near infrared VVV data

... Tauri and peculiar W ...days), and RVTs (P > 20 days). The thresholds are those by Soszy´nski et ...on the period distribu- tion of OGLE III T2Cs, and the authors kept ... See full document

11

Near infrared photometry of Galactic planetary nebulae with the VVV Survey

Near infrared photometry of Galactic planetary nebulae with the VVV Survey

... luminous and short-lived products of evolved low-mass stars ...). The stars eject much of their envelopes during a phase of strong mass loss at the end of ... See full document

10

Confirmation of a New Metal poor Globular Cluster in the Galactic Bulge

Confirmation of a New Metal poor Globular Cluster in the Galactic Bulge

... deep near-IR photometry of the VISTA Variables in the Vía Láctea ( VVV ) Survey and deep DECam Plane Survey ( DECaPS ) optical photometry to con fi rm the physical ... See full document

12

Chemical Abundances of the Highly Obscured Galactic Globular Clusters 2MASS GC02 and Mercer 5

Chemical Abundances of the Highly Obscured Galactic Globular Clusters 2MASS GC02 and Mercer 5

... images and low-resolution K-band spectra. Based on the analysis of the J Ks versus Ks color – magnitude diagram and spectroscopi- cally derived metallicities and radial ... See full document

11

A deep near infrared view of the Galactic globular cluster 2 MASS GC 02

A deep near infrared view of the Galactic globular cluster 2 MASS GC 02

... metal-rich globular cluster with a rel- atively high radial ...but the cluster does contain at least five RR Lyrae ...Interestingly, the periods of the fundamental-mode ... See full document

7

Milky Way demographics with the VVV survey II  Color transformations and near infrared photometry for 136 million stars in the southern Galactic disk

Milky Way demographics with the VVV survey II Color transformations and near infrared photometry for 136 million stars in the southern Galactic disk

... explore the variation of the transformation coefficients across single ...Each of these 64 sub-fields (1597 ×1957 pixels) was used to calculate the transformation coefficients with ... See full document

22

Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies

Mid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxies

... with the target being placed at six positions (separated by 20 ) along the slit using multiple cycles of the longest ramp setting of 120 s to maximize S/N in unit time, while ensuring ... See full document

18

Estimating the parameters of globular cluster M 30 (NGC 7099) from time series photometry

Estimating the parameters of globular cluster M 30 (NGC 7099) from time series photometry

... recover the first three known RR Lyrae in this clus- ter (V1-V3) in our data, and calculate periods for each of them, using phase dispersion minimisation (PDM; Stellingwerf 1978) and ... See full document

15

Low-Resolution Spectroscopy and uvby&beta Photometry of Selected Stars in Haffner 18

Low-Resolution Spectroscopy and uvby&beta Photometry of Selected Stars in Haffner 18

... tracings of the resulting spectrograms of the O-stars found here are shown in Figure ...in the MK system by identifying the photospheric lines present in its spectrogram using ... See full document

8

Optical photometry and spectroscopy of the 1987A like supernova 2009mw

Optical photometry and spectroscopy of the 1987A like supernova 2009mw

... comparison of SN 2009mw with other 1987A-like SNe shows that, while some of their parameters show differences, others such as their spectra, progenitors and environments are quite simi- ...sample ... See full document

11

EXTENSIVE SPECTROSCOPY AND PHOTOMETRY OF THE TYPE IIP SUPERNOVA 2013ej

EXTENSIVE SPECTROSCOPY AND PHOTOMETRY OF THE TYPE IIP SUPERNOVA 2013ej

... , and Hungarian OTKA grant NN 107637 ( ...Astronomy and Astrophysics Postdoc- toral Fellowship under award ...by the Lendület-2009 program of the Hungarian Academy of Sciences ... See full document

26

TIME SERIES PHOTOMETRY OF GLOBULAR CLUSTERS: M62 (NGC 6266), THE MOST RR LYRAE RICH GLOBULAR CLUSTER IN THE GALAXY?

TIME SERIES PHOTOMETRY OF GLOBULAR CLUSTERS: M62 (NGC 6266), THE MOST RR LYRAE RICH GLOBULAR CLUSTER IN THE GALAXY?

... Observations of the standard fields PG+0918, PG+1323, PG+1525, PG+1528, PG+1633, PG+1657, and Ru 152 (Landolt 1992) were obtained on the same nights, to calibrate the data to the ... See full document

21

Optical and infrared photometry of globular clusters in NGC 1399: Evidence for color metallicity nonlinearity

Optical and infrared photometry of globular clusters in NGC 1399: Evidence for color metallicity nonlinearity

... importance of the form of the color–metallicity relation on the one hand, and structure in the underlying metal- licity distribution on the other hand, remains an ... See full document

15

The Optical and Near-Infrared Counterpart of
IRAS 18476+2054

The Optical and Near-Infrared Counterpart of IRAS 18476+2054

... star and heats the dust to unusual high tem- peratures (Whitelock 1985; Corradi & Schwarz 1993, ...In the 2MASS data base (Cutri et al. 2000) it is given just at the overexposure ... See full document

6

VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies

VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies

... observations of globular clusters (GCs) in five low surface brightness dwarf galaxies: KK 211 and KK 221, both dwarf spheroidal satellites (dSph) of NGC 5128; dSph KK 84 located close ... See full document

18

The HST/ACS coma cluster survey  IV  Intergalactic globular clusters and the massive globular cluster system at the core of the coma galaxy cluster

The HST/ACS coma cluster survey IV Intergalactic globular clusters and the massive globular cluster system at the core of the coma galaxy cluster

... Coma cluster of galaxies (Abell 1656) is one of the nearest rich, dense clusters, and is a fundamental target for extragalactic ...Studies of GC systems in Coma from ... See full document

16

Estimation of density, moisture content and strength properties of Tectona grandis wood using near infrared spectroscopy

Estimation of density, moisture content and strength properties of Tectona grandis wood using near infrared spectroscopy

... Estimation of the mechanical properties of wood from Eucalyptus urophylla using near infrared. 371[r] ... See full document

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