Calendar

Oct
17
Wed
Astr110 Observatory
Oct 17 @ 9:00 pm – 10:00 pm
Oct
22
Mon
Astr110 Observatory
Oct 22 @ 9:00 pm – 10:00 pm
Oct
24
Wed
Astr110 Observatory
Oct 24 @ 9:00 pm – 10:00 pm
Oct
29
Mon
Astr110 Observatory
Oct 29 @ 9:00 pm – 10:00 pm
Oct
31
Wed
Astr110 Observatory
Oct 31 @ 9:00 pm – 10:00 pm
Nov
5
Mon
Astr110 Observatory
Nov 5 @ 9:00 pm – 10:00 pm
Nov
7
Wed
Astr110 Observatory
Nov 7 @ 9:00 pm – 10:00 pm
Nov
12
Mon
Astr110 Observatory
Nov 12 @ 9:00 pm – 10:00 pm
Nov
14
Wed
Astr110 Observatory
Nov 14 @ 9:00 pm – 10:00 pm
Jan
23
Wed
Colloquium Thesis Defense: Lauren Kahre
Jan 23 @ 3:00 pm – 4:00 pm
Colloquium Thesis Defense: Lauren Kahre

Extinction Mapping and Dust-to-Gas Ratios of Nearby Galaxies

Lauren Kahre, NMSU

We present a study of the dust{to{gas ratios in 31 nearby (D >
10 Mpc) galaxies. Using Hubble Space Telescope broad band WFC3/UVIS UV and
optical images from the Treasury program LEGUS (Legacy ExtraGalactic UV
Survey) combined with archival HST/ACS data, we correct thousands of
individual stars for extinction across these galaxies using an
isochrone-matching (reddening-free Q) method. We generate extinction maps
for each galaxy from the individual stellar extinctions using both
adaptive and fixed resolution techniques, and correlate these maps with
neutral HI and CO gas maps from literature, including The HI Nearby Galaxy
Survey (THINGS) and the HERA CO-Line ExtraGalactic Survey (HERACLES). We
calculate dust-to-gas ratios and investigate variations in the dust-to-gas
ratio with galaxy metallicity. We find a power law relationship between
dust-to-gas ratio and metallicity. The single power law is consistent with
other studies of dust-to-gas ratio compared to metallicity, while the
broken power law shows a significantly shallower slope for low metallicity
galaxies than previously observed. We find a change in the relation when
H_2 is not included. This implies that underestimation of N_H2 in
low-metallicity dwarfs from a too-low CO-to-H2 conversion factor X_CO
could have produced too low a slope in the derived relationship between
dust-to-gas ratio and metallicity. We also
compare our extinctions to those derived from fitting the spectral energy
distribution (SED) using the Bayesian Extinction and Stellar Tool (BEAST)
for NGC 7793 and and systematically lower extinctions from SED-fitting as
compared to isochrone matching. Finally, we compare our extinction maps of
NGC 628 to maps of the dust obtained via IR emission from Aniano et al.
(2012) and find a factor of 2 difference in dust-to-gas ratios determined
from the two maps, consistent with previous work.