We used optical images acquired with the UVIS channel of the Wide Field Camera 3 on board the Hubble Space Telescope to construct the first high-resolution extinction map in the direction of NGC 6440, a globular cluster located in the bulge of our Galaxy. The map has a spatial resolution of 0.″5 over a rectangular region of about 160″ × 240″ around the cluster center, with the long side in the northwest/southeast direction. We found that the absorption clouds show patchy and filamentary substructures with extinction variations as large as δE(B-V) ∼0.5 mag. We also performed a first-order proper motion analysis to distinguish cluster members from field interlopers. After the field decontamination and the differential reddening correction, the cluster sequences in the color-magnitude diagram appear much better defined, providing the best optical color-magnitude diagram so far available for this cluster.

Pallanca C., Ferraro F.R., Lanzoni B., Saracino S., Raso S., Focardi P. (2019). High-resolution Extinction Map in the Direction of the Bulge Globular Cluster NGC 6440. THE ASTROPHYSICAL JOURNAL, 882(2), 1-10 [10.3847/1538-4357/ab35db].

High-resolution Extinction Map in the Direction of the Bulge Globular Cluster NGC 6440

Pallanca C.
;
Ferraro F. R.
Funding Acquisition
;
Lanzoni B.;Raso S.;Focardi P.
2019

Abstract

We used optical images acquired with the UVIS channel of the Wide Field Camera 3 on board the Hubble Space Telescope to construct the first high-resolution extinction map in the direction of NGC 6440, a globular cluster located in the bulge of our Galaxy. The map has a spatial resolution of 0.″5 over a rectangular region of about 160″ × 240″ around the cluster center, with the long side in the northwest/southeast direction. We found that the absorption clouds show patchy and filamentary substructures with extinction variations as large as δE(B-V) ∼0.5 mag. We also performed a first-order proper motion analysis to distinguish cluster members from field interlopers. After the field decontamination and the differential reddening correction, the cluster sequences in the color-magnitude diagram appear much better defined, providing the best optical color-magnitude diagram so far available for this cluster.
2019
Pallanca C., Ferraro F.R., Lanzoni B., Saracino S., Raso S., Focardi P. (2019). High-resolution Extinction Map in the Direction of the Bulge Globular Cluster NGC 6440. THE ASTROPHYSICAL JOURNAL, 882(2), 1-10 [10.3847/1538-4357/ab35db].
Pallanca C.; Ferraro F.R.; Lanzoni B.; Saracino S.; Raso S.; Focardi P.
File in questo prodotto:
File Dimensione Formato  
11585_725438.pdf

accesso aperto

Tipo: Versione (PDF) editoriale
Licenza: Licenza per accesso libero gratuito
Dimensione 14.85 MB
Formato Adobe PDF
14.85 MB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/725438
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 13
  • ???jsp.display-item.citation.isi??? 14
social impact